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Journal articles on the topic 'Astrochemistry'

Author: Grafiati

Published: 4 June 2021

Last updated: 25 July 2025

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1

Millar, T. J. "Astrochemistry." Plasma Sources Science and Technology 24, no. 4 (2015): 043001. http://dx.doi.org/10.1088/0963-0252/24/4/043001.

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2

Brown, Wendy A. "Astrochemistry." Physical Chemistry Chemical Physics 16, no. 8 (2014): 3343. http://dx.doi.org/10.1039/c4cp90004a.

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3

Lepp, Stephen. "Astrochemistry revealed." Nature 379, no. 6566 (1996): 596. http://dx.doi.org/10.1038/379596a0.

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4

Wilson, T. L., and W. Batrla. "Radio Astrochemistry." EAS Publications Series 15 (2005): 331–45. http://dx.doi.org/10.1051/eas:2005161.

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5

Herbst, Eric, and John T. Yates. "Introduction: Astrochemistry." Chemical Reviews 113, no. 12 (2013): 8707–9. http://dx.doi.org/10.1021/cr400579y.

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6

Irvine, W. M., and Å. Hjalmarson. "Observational astrochemistry." Advances in Space Research 6, no. 12 (1986): 227–36. http://dx.doi.org/10.1016/0273-1177(86)90090-6.

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7

Indriolo, Nick, and Benjamin J. McCall. "Cosmic-ray astrochemistry." Chemical Society Reviews 42, no. 19 (2013): 7763. http://dx.doi.org/10.1039/c3cs60087d.

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8

Richards, A. "Astrochemistry of Life." Astronomy & Geophysics 42, no. 3 (2001): 3.5. http://dx.doi.org/10.1093/astrog/42.3.3.5.

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9

Dalgarno, Alexander. "Astrochemistry: A Summary." Proceedings of the International Astronomical Union 1, S231 (2006): 515. http://dx.doi.org/10.1017/s1743921306007551.

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10

Dalgarno, A. "Astrochemistry — A Summary." Symposium - International Astronomical Union 120 (1987): 577–81. http://dx.doi.org/10.1017/s0074180900154646.

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11

Tielens, A. G. G. M. "Diffuse Interstellar Bands: The Way Forward." Proceedings of the International Astronomical Union 9, S297 (2013): 399–411. http://dx.doi.org/10.1017/s1743921313016207.

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AbstractRather than a summary of the conference, I present here an overview of the status of the field and our progress over the last two decades from the points of view of astronomy, molecular physics, spectroscopy, and astrochemistry. While at first sight, progress may seem slow, actually, we have made an important stride forward. We have recognized now that the problem is very complex and identifying the carriers of the Diffuse Interstellar Bands will require a concerted effort of astronomers, molecular physicists, spectroscopists, and astrochemists. While this is a daunting prospect, we ha

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12

Prasad, Sheo S., and Pradip Gangopadhaya. "Astrochemistry Library with Artificial Intelligence for Quality Control." Symposium - International Astronomical Union 150 (1992): 19–20. http://dx.doi.org/10.1017/s0074180900089610.

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Libraries of reactions used in astrochemistry modeling have seen an explosive increase in size in recent years. Their quality control by manual effort is almost impossible. Expert systems with artificial intelligence are now needed to ensure the quality of large scale astrochemistry libraries.

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13

Min, Y. C. "ASTROCHEMISTRY AND INTERSTELLAR MOLECULES." Publications of The Korean Astronomical Society 25, no. 1 (2010): 1–13. http://dx.doi.org/10.5303/pkas.2010.25.1.001.

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14

Baker, J. "ASTROCHEMISTRY: Capturing Ferroelectric Ice." Science 315, no. 5808 (2007): 18b. http://dx.doi.org/10.1126/science.315.5808.18b.

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15

Peeters, Z., S. D. Rodgers, S. B. Charnley, et al. "Astrochemistry of dimethyl ether." Astronomy & Astrophysics 445, no. 1 (2005): 197–204. http://dx.doi.org/10.1051/0004-6361:20053651.

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16

Frankland, V. L., A. Rosu-Finsen, J. Lasne, M. P. Collings, and M. R. S. McCoustra. "Laboratory surface astrochemistry experiments." Review of Scientific Instruments 86, no. 5 (2015): 055103. http://dx.doi.org/10.1063/1.4919657.

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17

Richards, Anita, and Peter Sarre. "The astrochemistry of life." Astronomy and Geophysics 42, no. 6 (2001): 6.17–6.18. http://dx.doi.org/10.1046/j.1468-4004.2001.42617.x.

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18

Shematovich, V. I. "Suprathermal particles in astrochemistry." Russian Chemical Reviews 88, no. 10 (2019): 1013–45. http://dx.doi.org/10.1070/rcr4882.

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19

van Dishoeck, Ewine F. "Astrochemistry: overview and challenges." Proceedings of the International Astronomical Union 13, S332 (2017): 3–22. http://dx.doi.org/10.1017/s1743921317011528.

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AbstractThis paper provides a brief overview of the journey of molecules through the Cosmos, from local diffuse interstellar clouds and PDRs to distant galaxies, and from cold dark clouds to hot star-forming cores, protoplanetary disks, planetesimals and exoplanets. Recent developments in each area are sketched and the importance of connecting astronomy with chemistry and other disciplines is emphasized. Fourteen challenges for the field of Astrochemistry in the coming decades are formulated.

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20

Williams, David A. "Future Directions in Astrochemistry." Proceedings of the International Astronomical Union 1, S231 (2006): 521. http://dx.doi.org/10.1017/s1743921306007563.

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21

Rowe, B. R. "Chemical Reactions in Astrochemistry." Symposium - International Astronomical Union 150 (1992): 7–12. http://dx.doi.org/10.1017/s0074180900089579.

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This paper is devoted to chemistry in the gas phase dealing firstly with ion-molecule reactions at extremely low temperature. The experimental techniques that have been used in this field are shortly presented and the reactions that have been studied using the CRESU(S) method reviewed. In the second part, the most recent measurements concerning dissociative recombination are discussed, including studies of branching ratio and new determination of the rate coefficient for H+3 ions.

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22

Irvine, W. M. "Observational astrochemistry: Recent results." Advances in Space Research 9, no. 2 (1989): 3–12. http://dx.doi.org/10.1016/0273-1177(89)90357-8.

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23

Wlodarczak, G. "Rotational spectroscopy and astrochemistry." Journal of Molecular Structure 347 (March 1995): 131–42. http://dx.doi.org/10.1016/0022-2860(95)08541-3.

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24

Wakelam, V., and the Kida team. "Kinetic database for astrochemistry." EAS Publications Series 58 (2012): 287–90. http://dx.doi.org/10.1051/eas/1258047.

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25

Fortenberry, Ryan C. "Special issue: Computational astrochemistry." International Journal of Quantum Chemistry 117, no. 2 (2016): 80. http://dx.doi.org/10.1002/qua.25322.

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26

Ariana Remmel. "Looking beyond carbon in astrochemistry." C&EN Global Enterprise 100, no. 30 (2022): 5. http://dx.doi.org/10.1021/cen-10030-scicon2.

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27

Widicus Weaver, Susanna L. "Astrochemistry in the terahertz gap." Physics Today 75, no. 2 (2022): 28–33. http://dx.doi.org/10.1063/pt.3.4939.

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28

Talbi, D. "Theoretical approaches for studying Astrochemistry." EPJ Web of Conferences 18 (2011): 02002. http://dx.doi.org/10.1051/epjconf/20111802002.

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29

Williams, David A., and Serena Viti. "4 Recent progress in astrochemistry." Annu. Rep. Prog. Chem., Sect. C: Phys. Chem. 98 (2002): 87–120. http://dx.doi.org/10.1039/b111165p.

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30

Cridland, Alexander J., Christian Eistrup, and Ewine F. van Dishoeck. "Connecting planet formation and astrochemistry." Astronomy & Astrophysics 627 (July 2019): A127. http://dx.doi.org/10.1051/0004-6361/201834378.

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Combining a time-dependent astrochemical model with a model of planet formation and migration, we compute the carbon-to-oxygen ratio (C/O) of a range of planetary embryos starting their formation in the inner solar system (1–3 AU). Most of the embryos result in hot Jupiters (M ≥ MJ, orbital radius <0.1 AU) while the others result in super-Earths at wider orbital radii. The volatile and ice abundance of relevant carbon and oxygen bearing molecular species are determined through a complex chemical kinetic code that includes both gas and grain surface chemistry. This is combined with a model f

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31

Smith, Ian W. M. "Laboratory Astrochemistry: Gas-Phase Processes." Annual Review of Astronomy and Astrophysics 49, no. 1 (2011): 29–66. http://dx.doi.org/10.1146/annurev-astro-081710-102533.

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32

Cridland, Alex J., Ewine F. van Dishoeck, Matthew Alessi, and Ralph E. Pudritz. "Connecting planet formation and astrochemistry." Astronomy & Astrophysics 632 (November 28, 2019): A63. http://dx.doi.org/10.1051/0004-6361/201936105.

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To understand the role that planet formation history has on the observable atmospheric carbon-to-oxygen ratio (C/O) we have produced a population of astrochemically evolving protoplanetary disks. Based on the parameters used in a pre-computed population of growing planets, their combination allows us to trace the molecular abundances of the gas that is being collected into planetary atmospheres. We include atmospheric pollution of incoming (icy) planetesimals as well as the effect of refractory carbon erosion noted to exist in our own solar system. We find that the carbon and oxygen content of

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33

Cridland, Alex J., Ewine F. van Dishoeck, Matthew Alessi, and Ralph E. Pudritz. "Connecting planet formation and astrochemistry." Astronomy & Astrophysics 642 (October 2020): A229. http://dx.doi.org/10.1051/0004-6361/202038767.

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The chemical composition of planetary atmospheres has long been thought to store information regarding where and when a planet accretes its material. Predicting this chemical composition theoretically is a crucial step in linking observational studies to the underlying physics that govern planet formation. As a follow-up to an earlier study of ours on hot Jupiters, we present a population of warm Jupiters (semi-major axis between 0.5 and 4 AU) extracted from the same planetesimal formation population synthesis model as used in that previous work. We compute the astrochemical evolution of the p

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34

Millar, T. J., C. M. Walmsley, C. Rebrion-Rowe, L. d'Hendecourt, S. Saito, and F. Rostas. "Molecular Data Needs in Astrochemistry." Symposium - International Astronomical Union 197 (2000): 303–14. http://dx.doi.org/10.1017/s0074180900164897.

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The development of astrochemistry is inextricably linked to the generation of fundamental data. In this report, we discuss data needs in terms of astrochemical models, gas-phase kinetics, molecular excitation, optical and UV spectroscopy, solid-state chemistry, and millimeter and submillimeter wave spectroscopy.

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35

Hudson, Reggie L. "Astrochemistry Examples in the Classroom." Journal of Chemical Education 83, no. 11 (2006): 1611. http://dx.doi.org/10.1021/ed083p1611.

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36

Herbst, Eric. "The astrochemistry of H 3 +." Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences 358, no. 1774 (2000): 2523–34. http://dx.doi.org/10.1098/rsta.2000.0665.

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37

Williams, David A. "Introductory Lecture Frontiers of astrochemistry." Faraday Discussions 109 (1998): 1–14. http://dx.doi.org/10.1039/a804023k.

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38

Toscano, Jutta. "Rotational-state-selected Carbon Astrochemistry." CHIMIA 78, no. 1/2 (2024): 40–44. http://dx.doi.org/10.2533/chimia.2024.40.

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The addition of individual quanta of rotational excitation to a molecule has been shown to markedly change its reactivity by significantly modifying the intermolecular interactions. So far, it has only been possible to observe these rotational effects in a very limited number of systems due to lack of rotational selectivity in chemical reaction experiments. The recent development of rotationally controlled molecular beams now makes such investigations possible for a wide range of systems. This is particularly crucial in order to understand the chemistry occurring in the interstellar medium, su

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39

Puzzarini, Cristina, and Vincenzo Barone. "The challenging playground of astrochemistry: an integrated rotational spectroscopy – quantum chemistry strategy." Physical Chemistry Chemical Physics 22, no. 12 (2020): 6507–23. http://dx.doi.org/10.1039/d0cp00561d.

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40

Fioroni, Marco, Robert E. Savage, and Nathan J. DeYonker. "On the formation of phosphorous polycyclic aromatics hydrocarbons (PAPHs) in astrophysical environments." Physical Chemistry Chemical Physics 21, no. 15 (2019): 8015–21. http://dx.doi.org/10.1039/c9cp00547a.

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41

Bellili, A., Z. Gouid, M. C. Gazeau, et al. "Single photon ionization of methyl isocyanide and the subsequent unimolecular decomposition of its cation: experiment and theory." Physical Chemistry Chemical Physics 21, no. 47 (2019): 26017–26. http://dx.doi.org/10.1039/c9cp04310a.

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42

Ceccarelli, Cecilia, and Claudio Codella. "A shocking beginning to star formation." Physics Today 77, no. 5 (2024): 36–42. http://dx.doi.org/10.1063/pt.vkew.bmgd.

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43

Fioroni, Marco. "Astrochemistry of transition metals? The selected cases of [FeN]+, [FeNH]+ and [(CO)2FeN]+: pathways toward CH3NH2 and HNCO." Phys. Chem. Chem. Phys. 16, no. 44 (2014): 24312–22. http://dx.doi.org/10.1039/c4cp03218g.

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44

White, Douglas W. "Building an Astrophysics/Astrochemistry Laboratory fromScratch." Physics Teacher 60, no. 5 (2022): 362–64. http://dx.doi.org/10.1119/10.0010394.

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Laboratory astrophysics and astrochemistry are emerging fields highlighting the importance of laboratory simulations and experiments to benefit remote observations. In particular, ice mixtures found in the outer solar system may offer insight into the early evolution of organic molecules. H2O-ice mixtures containing other species such as NH3, CH3OH, CH4, CO2, etc. also provide interesting research avenues to explore via IR absorption spectroscopy towards building a laboratory database astronomers can use. As such, the astrochemistry laboratory at USC Aiken strives to fill this niche while fost

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45

McElroy, D., C. Walsh, A. J. Markwick, M. A. Cordiner, K. Smith, and T. J. Millar. "The UMIST database for astrochemistry 2012." Astronomy & Astrophysics 550 (January 22, 2013): A36. http://dx.doi.org/10.1051/0004-6361/201220465.

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46

Albertsson, Tobias, Jens Kauffmann, and Karl M. Menten. "Atlas of Cosmic-Ray-induced Astrochemistry." Astrophysical Journal 868, no. 1 (2018): 40. http://dx.doi.org/10.3847/1538-4357/aae775.

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47

Szuromi, P. D. "ASTROCHEMISTRY: Phenyl Radicals Over the Radio." Science 300, no. 5628 (2003): 2007c—2007. http://dx.doi.org/10.1126/science.300.5628.2007c.

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48

Baker, J. "ASTROCHEMISTRY: The Sun Reflected in Osbornite." Science 315, no. 5817 (2007): 1339d—1341d. http://dx.doi.org/10.1126/science.315.5817.1339d.

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49

Woodall, J., M. Agúndez, A. J. Markwick-Kemper, and T. J. Millar. "The UMIST database for astrochemistry 2006." Astronomy & Astrophysics 466, no. 3 (2007): 1197–204. http://dx.doi.org/10.1051/0004-6361:20064981.

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50

Jørgensen, Jes K., Arnaud Belloche, and Robin T. Garrod. "Astrochemistry During the Formation of Stars." Annual Review of Astronomy and Astrophysics 58, no. 1 (2020): 727–78. http://dx.doi.org/10.1146/annurev-astro-032620-021927.

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Star-forming regions show a rich and varied chemistry, including the presence of complex organic molecules—in both the cold gas distributed on large scales and the hot regions close to young stars where protoplanetary disks arise. Recent advances in observational techniques have opened new possibilities for studying this chemistry. In particular, the Atacama Large Millimeter/submillimeter Array has made it possible to study astrochemistry down to Solar System–size scales while also revealing molecules of increasing variety and complexity. In this review, we discuss recent observations of the c

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