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Journal articles on the topic 'Complex organic molecules'

Author: Grafiati

Published: 10 March 2023

Last updated: 26 July 2025

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1

Herbst, Eric, and Ewine F. van Dishoeck. "Complex Organic Interstellar Molecules." Annual Review of Astronomy and Astrophysics 47, no. 1 (2009): 427–80. http://dx.doi.org/10.1146/annurev-astro-082708-101654.

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Öberg, Karin I., Edith C. Fayolle, John B. Reiter, and Claudia Cyganowski. "Complex molecule formation around massive young stellar objects." Faraday Discuss. 168 (2014): 81–101. http://dx.doi.org/10.1039/c3fd00146f.

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Interstellar complex organic molecules were first identified in the hot inner regions of massive young stellar objects (MYSOs), but have more recently been found in many colder sources, indicating that complex molecules can form at a range of temperatures. However, individually these observations provide limited constraints on how complex molecules form, and whether the same formation pathways dominate in cold, warm and hot environments. To address these questions, we use spatially resolved observations from the Submillimeter Array of three MYSOs together with mostly unresolved literature data

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Soma, Tatsuya, Nami Sakai, Yoshimasa Watanabe, and Satoshi Yamamoto. "Complex Organic Molecules in Taurus Molecular Cloud-1." Astrophysical Journal 854, no. 2 (2018): 116. http://dx.doi.org/10.3847/1538-4357/aaa70c.

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Dartois, E., M. Chabot, T. Id Barkach, et al. "Non-thermal desorption of complex organic molecules." Astronomy & Astrophysics 627 (July 2019): A55. http://dx.doi.org/10.1051/0004-6361/201834787.

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Context. The occurrence of complex organic molecules (COMs) in the gas phase at low temperature in the dense phases of the interstellar medium suggests that a non-thermal desorption mechanism is at work because otherwise, COMs should condense within a short timescale onto dust grains. Vacuum ultraviolet (VUV) photodesorption has been shown to be much less efficient for complex organic molecules, such as methanol, because mostly photoproducts are ejected. The induced photolysis competes with photodesorption for large COMs, which considerably lowers the efficiency to desorb intact molecules. Aim

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5

Cruikshank, D. P. "Complex Organic Solid Matter in the Outer Solar System." Highlights of Astronomy 13 (2005): 902–3. http://dx.doi.org/10.1017/s1539299600017482.

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Complex organic molecular material of non-biological origin is found in abundance in the interstellar dust in our Galaxy, and is also detected in other galaxies. Some of this material was incorporated into the solar nebula and is now found in some Solar System bodies. While some pre-solar organic material has been preserved, synthesis of complex organics in planetary atmospheres and on icy surfaces has been in progress for the entire age of the Solar System. Refractory organic solids have proven difficult to detect by traditional spectroscopic techniques, and their presence is usually inferred

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Natalia, Inostroza-Pino. "Methanediol CH2(OH)2 and hydroxymethyl CH2OH+: key organic intermediates on the path to complex organic molecules." Astronomy & astrophysics A&A 664, A85 (2022) 664 (May 24, 2022): A85. https://doi.org/10.1051/0004-6361/202243520.

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Ab initio molecular dynamics simulations were carried out to study the formation pathways to complex organic molecules when a OH+ projectile hit a dust grain covered only by methanol molecules. The selected target material is a methanol cluster formed by ten units (CH3OH)10.The focus of this paper is the process where methanediol CH2(OH)2 and hydroxymethyl CH2OH+, both key organic intermediate molecules, were involved in the formation mechanisms of stable complex organic molecules (COMs).

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Walsh, Catherine, Tom J. Millar, Hideko Nomura, et al. "Complex organic molecules in protoplanetary disks." Astronomy & Astrophysics 563 (February 28, 2014): A33. http://dx.doi.org/10.1051/0004-6361/201322446.

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8

Faure, Alexandre, Eric Josselin, Laurent Wiesenfeld, and Cecilia Ceccarelli. "Collisional excitation of complex organic molecules." Proceedings of the International Astronomical Union 4, S251 (2008): 137–38. http://dx.doi.org/10.1017/s1743921308021376.

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AbstractA major difficulty in modelling the infrared and (sub)millimeter spectra of gas-phase complex organic molecules is the lack of state-to-state collisional rate coefficients. Accurate quantum or classical scattering calculations for large polyatomic species are indeed computationally highly challenging, particularly when both rotation and low frequency vibrations such as bending and torsional modes are involved. We briefly present here an approximate approach to estimate and/or extrapolate rotational and rovibrational rates for polyatomic molecules with many degrees of freedom.

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9

Liu, Sheng-Yuan. "Interferometric Observations of Complex Organic Molecules." Proceedings of the International Astronomical Union 1, S231 (2006): 217. http://dx.doi.org/10.1017/s1743921306007216.

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10

Choudhury, R., P. Schilke, G. Stéphan, et al. "Evolution of complex organic molecules in hot molecular cores." Astronomy & Astrophysics 575 (February 25, 2015): A68. http://dx.doi.org/10.1051/0004-6361/201424499.

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Ceccarelli, Cecilia. "Organic molecules in protostellar environments." Proceedings of the International Astronomical Union 4, S251 (2008): 79–88. http://dx.doi.org/10.1017/s174392130802125x.

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AbstractThe sequence that brings matter from a molecular cloud to a fully developed star plus planetary system seems to be a unique and rich chemistry laboratory where, step by step, molecular complexity increases. During the cold pre-collapse phase, atoms and simple molecules, like CO, freeze out onto the dust grains, forming icy mantles. Reactions on the grain surfaces likely form hydrogenated molecules (notably H2O, CH4, H2CO, CH3OH, and NH3) and perhaps even more complex organic molecules. The hallmark of this era is the super-deuteration phenomenon, i. e. the abnormal enhancement of molec

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12

Abplanalp, Matthew J., Samer Gozem, Anna I. Krylov, Christopher N. Shingledecker, Eric Herbst, and Ralf I. Kaiser. "A study of interstellar aldehydes and enols as tracers of a cosmic ray-driven nonequilibrium synthesis of complex organic molecules." Proceedings of the National Academy of Sciences 113, no. 28 (2016): 7727–32. http://dx.doi.org/10.1073/pnas.1604426113.

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Complex organic molecules such as sugars and amides are ubiquitous in star- and planet-forming regions, but their formation mechanisms have remained largely elusive until now. Here we show in a combined experimental, computational, and astrochemical modeling study that interstellar aldehydes and enols like acetaldehyde (CH3CHO) and vinyl alcohol (C2H3OH) act as key tracers of a cosmic-ray-driven nonequilibrium chemistry leading to complex organics even deep within low-temperature interstellar ices at 10 K. Our findings challenge conventional wisdom and define a hitherto poorly characterized re

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13

Dartois, E., M. Chabot, A. Bacmann, P. Boduch, A. Domaracka, and H. Rothard. "Non-thermal desorption of complex organic molecules." Astronomy & Astrophysics 634 (February 2020): A103. http://dx.doi.org/10.1051/0004-6361/201936934.

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Aims. Methanol ice is embedded in interstellar ice mantles present in dense molecular clouds. We aim to measure the sputtering efficiencies starting from different ice mantles of varying compositions experimentally, in order to evaluate their potential impact on astrochemical models. The sputtering yields of complex organic molecules is of particular interest, since few mechanisms are efficient enough to induce a significant feedback to the gas phase. Methods. We irradiated ice film mixtures made of methanol and carbon dioxide of varying ratios with swift heavy ions in the electronic sputterin

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14

Farrow, T., R. A. Taylor, and V. Vedral. "Towards witnessing quantum effects in complex molecules." Faraday Discussions 184 (2015): 183–91. http://dx.doi.org/10.1039/c5fd00101c.

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Whether many-body objects like organic molecules can exhibit full quantum behaviour, including entanglement, is an open fundamental question. We present a generic theoretical protocol for entangling two organic molecules, such as dibenzoterrylene in anthracene. The availability of organic dye molecules with two-level energy structures characterised by sharp and intense emission lines are characteristics that position them favourably as candidates for quantum information processing technologies involving single-photons. Quantum entanglement can in principle be generated between several organic

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Dartois, E., M. Chabot, T. Id Barkach, et al. "Non-thermal desorption of complex organic molecules." Astronomy & Astrophysics 628 (August 2019): C2. http://dx.doi.org/10.1051/0004-6361/201834787e.

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16

Ohishi, Masatoshi. "Search for complex organic molecules in space." Journal of Physics: Conference Series 728 (July 2016): 052002. http://dx.doi.org/10.1088/1742-6596/728/5/052002.

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de, la Torre Bruno, Martin Švec, Prokop Hapala, et al. "Non-covalent control of spin-state in metal-organic complex by positioning on N-doped graphene." Nature Communications 9 (July 19, 2018): 2831. https://doi.org/10.1038/s41467-018-05163-y.

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Nitrogen doping of graphene significantly affects its chemical properties, which is particularly important in molecular sensing and electrocatalysis applications. However, detailed insight into interaction between N-dopant and molecules at the atomic scale is currently lacking. Here we demonstrate control over the spin state of a single iron(II) phthalocyanine molecule by its positioning on N-doped graphene. The spin transition was driven by weak intermixing between orbitals with z-component of N-dopant (pz of N-dopant) and molecule (dxz, dyz, dz 2) with subsequent reordering of the Fe d-orbit

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18

Fayolle, Edith C., Karin I. Öberg, Robin T. Garrod, Ewine F. van Dishoeck, and Suzanne E. Bisschop. "Complex organic molecules in organic-poor massive young stellar objects." Astronomy & Astrophysics 576 (March 25, 2015): A45. http://dx.doi.org/10.1051/0004-6361/201323114.

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Filho, Eloi Alves da Silva, Fabricio Uliana, Stêner Romanel Ambrozio, Cleverton Oliveira, Renan Martin, and Arlan da Silva Gonçalves. "COMPUTATIONAL STUDY OF ORGANIC COMPOUNDS – AN APPLICATION FOR LEARNING IN CHEMISTRY." Revista Ifes Ciência 5, no. 1 (2019): 257–66. http://dx.doi.org/10.36524/ric.v5i1.293.

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Organic chemistry is a theme not so easy to understand by undergraduating students. The motivation of this work was carried out computational study of three different molecules by molecular modeling using classic and semi-empirical methods besides open-source softwares. The optimized structures were visualized through 3D representations which made the study more understanding. Physical chemistry properties were extracted from all molecules. For the molecule one there was good correlation between the calculation methods. For the molecule two and more complex structures like molecule three and f

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20

Jain, Akash, Ilya A. Shkrob, and Rajeev S. Assary. "Synthesis-Driven Computational Discovery of Organic Redoxmers for Non-Aqueous Redox Flow Batteries." ECS Meeting Abstracts MA2023-01, no. 3 (2023): 724. http://dx.doi.org/10.1149/ma2023-013724mtgabs.

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Organic non-aqueous redox flow batteries (RFBs) are promising grid-scale energy storage systems for storing intermittent renewable energy in molecules. For practical applications, low-cost and stable redox active molecules (redoxmers) that display a large redox potential window and long electrochemical cycling stability are required to deliver a high-energy-density RFB with a long battery cycle life. To accelerate the discovery of redoxmer molecules, previous studies have utilized machine learning (ML) methods along with first-principles simulations. Although many ML-suggested molecules show p

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21

Veciana, Jaume, and Hiizu Iwamura. "Organic Magnets." MRS Bulletin 25, no. 11 (2000): 41–51. http://dx.doi.org/10.1557/mrs2000.223.

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The notion of organic molecular materials showing metallic properties, such as electric conductivity or ferromagnetism, started several decades ago as a mere dream of some members of the chemical community. The goal was to create an assembly of organic molecules or macromolecules containing only light elements (C, H, N, O, S, etc.) and yet possessing the electron/hole mobility or spin alignment that is inherent in typical metals or their oxides and different from the isolated molecular materials. Organic molecular conductors initially were developed during the 1960s, but the first examples of

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22

Steele, A., L. G. Benning, R. Wirth, et al. "Organic synthesis associated with serpentinization and carbonation on early Mars." Science 375, no. 6577 (2022): 172–77. http://dx.doi.org/10.1126/science.abg7905.

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Abiotic formation of organic molecules Mars rovers have found complex organic molecules in the ancient rocks exposed on the planet’s surface and methane in the modern atmosphere. It is unclear what processes produced these organics, with proposals including both biotic and abiotic sources. Steele et al . analyzed the nanoscale mineralogy of the Mars meteorite ALH 84001 and found evidence of organic synthesis driven by serpentinization and carbonation reactions that occurred during the aqueous alteration of basalt rock by hydrothermal fluids. The results demonstrate that abiotic production of o

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23

Weaver, Susanna L. Widicus, Robin T. Garrod, Jacob C. Laas, and Eric Herbst. "Models of Hot Cores with Complex Molecules." Proceedings of the International Astronomical Union 7, S280 (2011): 79–87. http://dx.doi.org/10.1017/s1743921311024884.

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AbstractRecent models of hot cores have incorporated previously-uninvestigated chemical pathways that lead to the formation of complex organic molecules (COMs; i.e. species containing six or more atoms). In addition to the gas-phase ion-molecule reactions long thought to dominate the organic chemistry in these regions, these models now include photodissociation-driven grain surface reaction pathways that can also lead to COMs. Here, simple grain surface ice species photodissociate to form small radicals such as OH, CH3, CH2OH, CH3O, HCO, and NH2. These species become mobile at temperatures abo

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Lee, Tsung-Hsun, Jhen-Hao Li, Wei-Shun Huang, et al. "Magnetoconductance responses in organic charge-transfer-complex molecules." Applied Physics Letters 99, no. 7 (2011): 073307. http://dx.doi.org/10.1063/1.3627170.

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25

Zeman, Ellen J. "Complex Organic Molecules Found in Interplanetary Dust Particles." Physics Today 47, no. 3 (1994): 17–19. http://dx.doi.org/10.1063/1.2808432.

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26

Álvarez-Barcia, S., P. Russ, J. Kästner, and T. Lamberts. "Hydrogen transfer reactions of interstellar complex organic molecules." Monthly Notices of the Royal Astronomical Society 479, no. 2 (2018): 2007–15. http://dx.doi.org/10.1093/mnras/sty1478.

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27

Kukhto, A. V. "Luminescence of complex organic molecules upon electron excitation." Journal of Applied Spectroscopy 65, no. 5 (1998): 722–38. http://dx.doi.org/10.1007/bf02679844.

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28

Bergner, Jennifer B., Karin I. Öberg, Robin T. Garrod, and Dawn M. Graninger. "Complex Organic Molecules toward Embedded Low-mass Protostars." Astrophysical Journal 841, no. 2 (2017): 120. http://dx.doi.org/10.3847/1538-4357/aa72f6.

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Cuadrado, S., J. R. Goicoechea, J. Cernicharo, A. Fuente, J. Pety, and B. Tercero. "Complex organic molecules in strongly UV-irradiated gas." Astronomy & Astrophysics 603 (July 2017): A124. http://dx.doi.org/10.1051/0004-6361/201730459.

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30

Philipp, Dean M., Mark A. Watson, Haoyu S. Yu, Thomas B. Steinbrecher, and Art D. Bochevarov. "Quantum chemical pKa prediction for complex organic molecules." International Journal of Quantum Chemistry 118, no. 12 (2017): e25561. http://dx.doi.org/10.1002/qua.25561.

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31

Rojas-García, O. S., A. I. Gómez-Ruiz, A. Palau, M. T. Orozco-Aguilera, M. Chavez Dagostino, and S. E. Kurtz. "Interstellar Complex Organic Molecules in SiO-traced Massive Outflows." Astrophysical Journal Supplement Series 262, no. 1 (2022): 13. http://dx.doi.org/10.3847/1538-4365/ac81cb.

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Abstract The interstellar medium contains dust and gas, in which molecules can proliferate at high densities and in cold conditions. Interstellar complex organic molecules (iCOMs) are C-bearing species that contain at least six atoms. As they are detected in young stellar objects, iCOMs are expected to inhabit early stages of star formation evolution. In this study, we try to determine which iCOMs are present in the outflow component of massive protostars. To do this, we analyzed the morphological extension of blue- and redshifted iCOM emission in a sample of 11 massive protostars employing ma

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32

Sagan, C., W. R. Thompson, and B. N. Khare. "Titan's Organic Chemistry." Symposium - International Astronomical Union 112 (1985): 107–21. http://dx.doi.org/10.1017/s007418090014642x.

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Voyager discovered nine simple organic molecules in the atmosphere of Titan. Complex organic solids, called tholins, produced by irradiation of simulated Titanian atmosphere are consistent with measured properties of Titan from ultraviolet to microwave frequencies, and are the likely main constituents of the observed red aerosols. The tholins contain many of the organic building blocks central to life on Earth. At least 100 m and possibly kms thickness of complex organics have been produced on Titan during the age of the solar system, and may exist today as submarine deposits beneath an extens

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Overman, Larry E. "Molecular rearrangements in the construction of complex molecules." Tetrahedron 65, no. 33 (2009): 6432–46. http://dx.doi.org/10.1016/j.tet.2009.05.067.

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34

Molina-Ontoria, Agustín, María Gallego, Luís Echegoyen, Emilio M. Pérez, and Nazario Martín. "Organic solar cells based on bowl-shaped small-molecules." RSC Advances 5, no. 40 (2015): 31541–46. http://dx.doi.org/10.1039/c5ra02073e.

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A supramolecular approach involving bowl-shape molecules as electron donors has been used for the preparation of small-molecule solar cells. The PCE values depend directly on the formation of the supramolecular complex.

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35

Nuevo, Michel, George Cooper, John M. Saunders, Christina E. Buffo, and Scott A. Sandford. "Formation of complex organic molecules in astrophysical environments: Sugars and derivatives." Proceedings of the International Astronomical Union 15, S350 (2019): 123–26. http://dx.doi.org/10.1017/s1743921319009323.

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AbstractCarbonaceous meteorites contain a large variety of complex organic molecules, including amino acids, nucleobases, sugar derivatives, amphiphiles, and other compounds of astrobiological interest. Photoprocessing of ices condensed on cold grains with ultraviolet (UV) photons was proposed as an efficient way to form such complex organics in astrophysical environments. This hypothesis was confirmed by laboratory experiments simulating photo-irradiation of ices containing H2O, CH3OH, CO, CO2, CH4, H2CO, NH3, HCN, etc., condensed on cold (~10–80 K) substrates. These experiments resulted in t

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Leroux, Killian, and Lahouari Krim. "Thermal and photochemical study of CH3OH and CH3OH–O2 astrophysical ices." Monthly Notices of the Royal Astronomical Society 500, no. 1 (2020): 1188–200. http://dx.doi.org/10.1093/mnras/staa3205.

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ABSTRACT Methanol, which is one of the most abundant organic molecules in the interstellar medium, plays an important role in the complex grain surface chemistry that is believed to be a source of many organic compounds. Under energetic processing such as ultraviolet (UV) photons or cosmic rays, methanol may decompose into CH4, CO2, CO, HCO, H2CO, CH3O and CH2OH, which in turn lead to complex organic molecules such as CH3OCHO, CHOCH2OH and HOCH2CH2OH through radical recombination reactions. However, although molecular oxygen and its detection, abundance and role in the interstellar medium have

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Ehrenfreund, Pascale, Marco Spaans, and Nils G. Holm. "The evolution of organic matter in space." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 369, no. 1936 (2011): 538–54. http://dx.doi.org/10.1098/rsta.2010.0231.

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Carbon, and molecules made from it, have already been observed in the early Universe. During cosmic time, many galaxies undergo intense periods of star formation, during which heavy elements like carbon, oxygen, nitrogen, silicon and iron are produced. Also, many complex molecules, from carbon monoxide to polycyclic aromatic hydrocarbons, are detected in these systems, like they are for our own Galaxy. Interstellar molecular clouds and circumstellar envelopes are factories of complex molecular synthesis. A surprisingly high number of molecules that are used in contemporary biochemistry on the

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38

Whittet, D. C. B. "Interstellar Dust and the Organic Inventories of Early Solar Systems." Symposium - International Astronomical Union 213 (2004): 163–68. http://dx.doi.org/10.1017/s0074180900193192.

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Interstellar dust grains are vectors for cosmic carbon and other biogenic chemical elements. They deliver carbon to protoplanetary disks in various refractory phases (amorphous, graphitic, etc.), and they are coated with icy mantles that contain organic molecules and water. The nature of the organics present in and on the dust appears to be closely related to physical conditions. Complex molecules may be synthesized when simple ices are irradiated. Astronomical observations show that this occurs in the vicinity of certain massive protostars, but it is not known whether our Solar System formed

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Sakai, Nami, and Satoshi Yamamoto. "Observations of Complex Molecules in Low-Mass Protostars." Proceedings of the International Astronomical Union 7, S280 (2011): 43–52. http://dx.doi.org/10.1017/s1743921311024859.

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AbstractLow-mass star forming regions are rich inventories of complex organic molecules. Furthermore, they show significant chemical diversity even among sources in a similar physical evolutionary stage (i.e. Class 0 sources). One distinct case is the hot corino chemistry characterized by rich existence of saturated complex organic molecules such as HCOOCH3 and C2H5CN, whereas the other is the warm carbon-chain chemistry (WCCC) characterized by extraordinary richness of unsaturated complex organic molecules such as carbon-chain molecules. We here summarize these observational achievements duri

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Bottinelli, Sandrine, Cecilia Ceccarelli, Roberto Neri, and Jonathan P. Williams. "High-resolution observations of CH3CN in the hot corino of NGC1333-IRAS4A." Proceedings of the International Astronomical Union 4, S251 (2008): 117–18. http://dx.doi.org/10.1017/s1743921308021303.

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AbstractThe formation and evolution of complex organic molecules in the early stages of solar-type protostars (Class 0 objects) is crucial as it sets the stage for the content in pre-biotic molecules of the subsequent proto-planetary nebula. In order to understand the chemistry of these Class 0 objects, it is necessary to perform interferometric observations which allow us to resolve the hot corino, that is the warm, dense inner region of the envelope of a Class 0 object, where the complex organic molecules are located. Such observations exist for only two objects so far, IRAS16293-2422 and NG

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Bottinelli, Sandrine, Adwin C. A. Boogert, Ewine F. van Dishoeck, et al. "Precursors of complex organic molecules: NH3 and CH3OH in the ices surrounding low-mass protostars." Proceedings of the International Astronomical Union 4, S251 (2008): 105–10. http://dx.doi.org/10.1017/s1743921308021285.

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AbstractNH3 and CH3OH are key molecules in the chemical networks leading to the formation of complex N- and O-bearing organic molecules. However, despite a number of recent studies, there is still a lot to learn about their abundances in the solid state and how they relate to those of other N/O-bearing organic molecules or to NH3 and CH3OH abundances in the gas phase. This is particularly true in the case of low-mass young stellar objects (YSOs), for which only the recent advent of the Spitzer Space Telescope has allowed high sensitivity observations of the ices in their enveloppes. We present

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Shaikh, Moniruzzaman, Xinyao Liu, Kasra Amini, Tobias Steinle, and Jens Biegert. "High density molecular jets of complex neutral organic molecules with Tesla valves." Review of Scientific Instruments 92, no. 10 (2021): 104103. http://dx.doi.org/10.1063/5.0060904.

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43

Belloche, A., H. S. P. Müller, R. T. Garrod, and K. M. Menten. "Exploring Molecular Complexity with ALMA: Deuterated complex organic molecules in Sgr B2." EAS Publications Series 75-76 (2015): 329–32. http://dx.doi.org/10.1051/eas/1575066.

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Basova, Tamara. "Organic/Inorganic Nanocomposites Based on ‘Three Pillars’ (Organic Compounds, Metal Nanoparticles, and Carbon Nanomaterials)." International Journal of Molecular Sciences 26, no. 14 (2025): 6578. https://doi.org/10.3390/ijms26146578.

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A wide variety of organic molecules, ranging from simple aromatic molecules to complexes with organic ligands and polymers, offer the possibility of creating both simple and complex structures with diverse physicochemical properties [...]

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45

Kalenskii, S. V., and E. A. Mikheeva. "SPECTRAL SURVEY OF THE STAR FORMATION REGION DR21OH IN THE 4-mm WAVELENGTH RANGE." Астрономический журнал 100, no. 12 (2023): 1162–89. http://dx.doi.org/10.31857/s0004629923120034.

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The results of a spectral survey of the star-forming region DR21OH in the 4 mm wavelength range are presented. Sixty-nine molecules and their isotopologues have been detected, ranging from simple diatomic or triatomic molecules, such as SO, SiO and CCH, to complex organic species, such as CH3OCHO or CH3OCH3. A noТаблица part of the results qualitatively repeat the results of the survey of the same source at 3 mm. The inventories of molecules found at 3 and 4 mm overlap to a great extent. However, at 4 mm we found a number of species that have no allowed transitions in the 3 mm wavelength range

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Kuan, Y. J., H. C. Huang, S. B. Charnley, et al. "Prebiologically Important Interstellar Molecules." Symposium - International Astronomical Union 213 (2004): 185–88. http://dx.doi.org/10.1017/s0074180900193246.

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Understanding the organic chemistry of molecular clouds, particularly the formation of biologically important molecules, is fundamental to the study of the processes which lead to the origin, evolution and distribution of life in the Galaxy. Determining the level of molecular complexity attainable in the clouds, and the nature of the complex organic material available to protostellar disks and the planetary systems that form from them, requires an understanding of the possible chemical pathways and is therefore a central question in astrochemistry. We have thus searched for prebiologically imp

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Мигович, М,, and В. Кельман. "Photophysical processes at UV irradiation of complex organic molecules." Scientific Herald of Uzhhorod University.Series Physics 35 (June 30, 2014): 156–61. http://dx.doi.org/10.24144/2415-8038.2014.35.156-161.

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Neumann, M. A. "Crystal structures of moderately complex organic molecules are predictable." Acta Crystallographica Section A Foundations of Crystallography 63, a1 (2007): s37—s38. http://dx.doi.org/10.1107/s0108767307099163.

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Neumann, M. A. "Crystal structures of moderately complex organic molecules are predictable." Acta Crystallographica Section A Foundations of Crystallography 64, a1 (2008): C205—C206. http://dx.doi.org/10.1107/s0108767308093409.

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Vastel, C., C. Ceccarelli, B. Lefloch, and R. Bachiller. "THE ORIGIN OF COMPLEX ORGANIC MOLECULES IN PRESTELLAR CORES." Astrophysical Journal 795, no. 1 (2014): L2. http://dx.doi.org/10.1088/2041-8205/795/1/l2.

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