Bibliografie tematiche / Astrophysical ices

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Letteratura scientifica selezionata sul tema "Astrophysical ices"

Autore: Grafiati
Pubblicato: 11 gennaio 2025
Ultima modifica: 28 luglio 2025

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Articoli di riviste sul tema "Astrophysical ices"

1

Palumbo, M. E., G. A. Baratta, D. Fulvio, et al. "Ion irradiation of astrophysical ices." Journal of Physics: Conference Series 101 (February 1, 2008): 012002. http://dx.doi.org/10.1088/1742-6596/101/1/012002.

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Palumbo, M. E., G. A. Baratta, G. Leto, and G. Strazzulla. "H bonds in astrophysical ices." Journal of Molecular Structure 972, no. 1-3 (2010): 64–67. http://dx.doi.org/10.1016/j.molstruc.2009.12.017.

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3

Boduch, Philippe, Emmanuel Dartois, Ana L. F. de Barros, et al. "Radiation effects in astrophysical ices." Journal of Physics: Conference Series 629 (July 13, 2015): 012008. http://dx.doi.org/10.1088/1742-6596/629/1/012008.

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Strazzulla, G., A. C. Castorina, and M. E. Palumbo. "Ion irradiation of astrophysical ices." Planetary and Space Science 43, no. 10-11 (1995): 1247–51. http://dx.doi.org/10.1016/0032-0633(95)00040-c.

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Farenzena, L. S., P. Iza, R. Martinez, et al. "Electronic Sputtering Analysis of Astrophysical Ices." Earth, Moon, and Planets 97, no. 3-4 (2005): 311–29. http://dx.doi.org/10.1007/s11038-006-9081-y.

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6

Golikov, O., D. Yerezhep, A. Akylbayeva, D. Sokolov, E. Korshikov, and A. Aldiyarov. "Cryovacuum facilities for studying astrophysical ices." Low Temperature Physics 50, no. 1 (2024): 66–72. http://dx.doi.org/10.1063/10.0023894.

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Abstract (sommario):
This work introduces a cryovacuum apparatus used to investigate substances under near-space conditions. This device allows one to study the refractive index, infrared spectra, and density of substances that are condensed from the vapor phase onto a cooled substrate at temperatures ranging from 11 K to 300 K. Concurrently, the ultimate pressure of 0.1 nTorr can be obtained in the vacuum chamber. The introduced setup utilizes FTIR spectroscopy with a spectral measurement range of 400–7800 cm−1 and laser interference needed to determine the important physical and optical parameters. Several exper
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Moore, Marla H., and Reggie L. Hudson. "Production of Complex Molecules in Astrophysical Ices." Proceedings of the International Astronomical Union 1, S231 (2006): 247. http://dx.doi.org/10.1017/s1743921306007241.

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Rocard, F., J. Bénit, J.-P. Bibrtng, D. Ledu, and R. Meunier. "Erosion of ices: Physical and astrophysical discussion." Radiation Effects 99, no. 1-4 (1986): 97–104. http://dx.doi.org/10.1080/00337578608209617.

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Strazzulla, G. "Crystalline and amorphous structure of astrophysical ices." Low Temperature Physics 39, no. 5 (2013): 430–33. http://dx.doi.org/10.1063/1.4807045.

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Förstel, M., P. Maksyutenko, B. M. Jones, B. J. Sun, A. H. H. Chang, and R. I. Kaiser. "Synthesis of urea in cometary model ices and implications for Comet 67P/Churyumov–Gerasimenko." Chemical Communications 52, no. 4 (2016): 741–44. http://dx.doi.org/10.1039/c5cc07635h.

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Tesi sul tema "Astrophysical ices"

1

Dissly, Richard W. Anicich Vincent G. Anicich Vincent G. Allen Mark Andrew. "Laboratory studies of astrophysical ices /." Diss., Pasadena, Calif. : California Institute of Technology, 1995. http://resolver.caltech.edu/CaltechETD:etd-10312007-083146.

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2

Dawes, Anita. "Spectroscopic study of photon, ion and electron stimulated molecular synthesis in astrophysical ices." Thesis, University College London (University of London), 2003. http://oro.open.ac.uk/40046/.

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Abstract (sommario):
The universe is a vast chemical and physical factory consisting of large collections of stars, gas and dust. Energetic processing of ices and subsequent molecular synthesis in astrophysical environments, including icy Solar System bodies and grain mantles in the interstellar medium, are responsible for the observation of some of the molecular species found in space. Gas phase processes alone cannot explain the reaction mechanisms and the observed abundances of some of these molecules. This thesis reviews the current state of knowledge on solid state molecular synthesis in astrophysical ices an
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Bychkova, Anna. "Energetic iοn prοcessing οf arοmatic mοlecules in the sοlid phase". Electronic Thesis or Diss., Normandie, 2024. http://www.theses.fr/2024NORMC236.

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Abstract (sommario):
Dans les nuages denses, les manteaux glacés sont des condensats de petites molécules sur des grains solides. Ces manteaux glacés représentent des sites prometteurs pour certains processus chimiques. Ils sont constamment irradiés et de nouvelles molécules organiques complexes peuvent être ainsi formées. Une fois que les nuages denses se transforment en disque d'accrétion et, éventuellement, en système planétaire, ces manteaux glacés peuvent potentiellement contribuer au réservoir de molécules complexes des planètes. Dans cette thèse, les effets de l'irradiation ionique sur deux molécules aromat
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Holtom, Philip Derek. "Irradiation studies of astrophysical ice analogues." Thesis, University College London (University of London), 2005. http://discovery.ucl.ac.uk/1444790/.

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In this thesis the formation of molecular species in cold icy mantles, typical of those in the interstellar medium (ISM) has been studied. The construction of an ultra high vacuum system for the formation and containment of these astrophysical ice analogues is described. The method of preparation of these ices is detailed and analysis methodologies are discussed. VUV spectra of molecular ices (e.g. SO2, CH3NH2, OCS) measured on the UV1 beam line of the Astrid Synchrotron facility at the University of Aarhus in Denmark, are presented. Molecular synthesis (e.g. CO3, CO, H2CO3) induced by ion irr
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Korsmeyer, Julie. "Anthracroronene in Astrophysical Water-Ice Analogs." Scholarship @ Claremont, 2019. https://scholarship.claremont.edu/scripps_theses/1413.

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Abstract (sommario):
Polycyclic aromatic hydrocarbons (PAHs) are the most abundant large organic molecules in space. They are thought to be the main contributor to the unidentified infrared (UIR) emission bands from the interstellar medium (ISM) for several reasons: UIR intensities correspond to carbon abundance, indicating the presence of a carbon-based molecule; UIRs are found in extremely harsh environments which means the source must be a stable molecule. The most important evidence is if the bands in mid-infrared (MIR) or 'fingerprint' region match those of PAHs. Through the infrared spectroscopy of matrix-is
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Ding, Jing-Jie. "Irradiation of water ice and astrophysical implication." Caen, 2014. http://www.theses.fr/2014CAEN2056.

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Abstract (sommario):
Les glaces sont présentes dans notre système solaire par exemple sur les comètes, les lunes de Jupiter et de Saturne ainsi que sur les objets trans-neptuniens. Dans le milieu interstellaire, ces glaces forment une fine couche à la surface de grains des nuages denses. L’eau (H2O) est la molécule la plus abondante dans ces glaces. Ces glaces sont constamment exposées aux rayons cosmiques, au vent solaire et aux ions piégés dans la magnétosphère des planètes géantes. Les simulations de ce type d’irradiation associées aux observations peuvent nous amener à comprendre la grande variété des processu
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7

Sanfélix, Maria Jose Cabrera. "Molecular modelling of water ice in atmospheric and astrophysical environments." Thesis, University of Liverpool, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.415664.

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8

Hettlage, Christian. "Lepton production in ice by scattering of astrophysical neutrinos at high energies." Doctoral thesis, [S.l.] : [s.n.], 2005. http://webdoc.sub.gwdg.de/diss/2005/hettlage.

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Muntean, E. A. "Low energy ion irradiation of astrophysical ice analogues : sputtering and molecule formation." Thesis, Queen's University Belfast, 2014. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.680064.

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Abstract (sommario):
The work presented in this thesis is an experimental investigation into the sputtering of oxygen and water ice by 4 ke V ions under conditions existing in the Interstellar Medium (ISM). This work is divided into two main parts : 1) sputtering of oxygen ice by singly and doubly charged ions He+, Ar+, C+, N+ ,0, C2+, N2+ and 0 2+ and 2) sputtering of water ice by C+, N+, 0+, C2+, N2+ and 0 2+. The experimental sputter yield obtained for both oxygen and water ice is compared with those from a theoretical obtained model and found to be in reasonable agreement within the experimental errors. For ox
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10

Dupuy, Rémi. "Photon and electron induced desorption from molecular ices Spectrally-resolved UV photodesorption of CH4 in pure and layered ices The efficient photodesorption of nitric oxide (NO) ices : a laboratory astrophysics study X-ray photodesorption from water ice in protoplanetary disks and X-ray-dominated regions." Thesis, Sorbonne université, 2019. http://www.theses.fr/2019SORUS068.

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Abstract (sommario):
L’excitation électronique de molécules condensées sur des surfaces froides (10-100 K) peut mener à la désorption de certaines de ces molécules. Ce processus fondamental a des conséquences dans de nombreuses disciplines, dont deux ont guidé ce travail : l’astrochimie et la dynamique du vide dans les accélérateurs. La désorption induite par photons et électrons est étudiée pour des films amorphes de molécules condensées (glaces) telles que CO, H2O, NO ou CH4. Un objectif de cette thèse est la quantification de la désorption des différentes espèces, et d’explorer les paramètres pouvant affecter l
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Libri sul tema "Astrophysical ices"

1

1939-, Klinger Jürgen, and North Atlantic Treaty Organization. Scientific Affairs Division., eds. Ices in the solar system. D. Reidel, 1985.

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2

B, Schmitt, Bergh C. de, and Festou M, eds. Solar system ices: Based on reviews presented at the international symposium "solar system ices" held in Toulouse, France, on March 27-30, 1995. Kluwer Academic Publishers, 1998.

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3

Gudipati, Murthy S. The Science of Solar System Ices. Springer New York, 2013.

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4

Calif.) The Science of Solar System Ices Workshop (2008 Oxnard. The Science of Solar System Ices (ScSSI): A cross-disciplinary workshop, May 5-8, 2008, Oxnard, California. Lunar and Planetary Institute, 2008.

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5

Poinsatte, Philip E. Convective heat transfer measurements from a NACA 0012 airfoil in flight and in the NASA Lewis icing research tunnel. NASA, 1990.

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Poinsatte, Philip E. Convective heat transfer measurements from a NACA 0012 airfoil in flight and in the NASA Lewis icing research tunnel. NASA, 1990.

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7

(Editor), B. Schmitt, C. de Bergh (Editor), and M. Festou (Editor), eds. Solar System Ices (Astrophysics and Space Science Library). Springer, 2007.

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8

Gudipati, Murthy S., and Julie Castillo-Rogez. Science of Solar System Ices. Springer New York, 2012.

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Gudipati, Murthy S., and Julie Castillo-Rogez. The Science of Solar System Ices. Springer, 2014.

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Gudipati, Murthy S., and Julie Castillo-Rogez. The Science of Solar System Ices. Springer, 2012.

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Capitoli di libri sul tema "Astrophysical ices"

1

Satorre, Miguel Ángel, Ramón Luna, Carlos Millán, Manuel Domingo, and Carmina Santonja. "Density of Ices of Astrophysical Interest." In Laboratory Astrophysics. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-90020-9_4.

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2

Muñoz Caro, Guillermo M., and Rafael Martín Doménech. "Photon-Induced Desorption Processes in Astrophysical Ices." In Laboratory Astrophysics. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-90020-9_9.

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Satorre, M. A., G. Blanes, M. A. Hernández, C. Millán, M. Domingo, and M. C. Santonja. "An Experimental Setup for the Characterization of Ices of Astrophysical Interest." In Highlights of Spanish Astrophysics II. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-017-1776-2_125.

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Luna, R., M. A. Satorre, G. Blanes, M. C. Santonja, M. Domingo, and O. Gomis. "Density Determination of Ices of Astrophysical Interest by Double-Laser Interferometry." In Highlights of Spanish Astrophysics III. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-1778-6_132.

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Pirronello, Valerio. "Physical and Chemical Effects Induced by Fast Ions in Ices of Astrophysical Interest." In Chemistry in Space. Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-009-0695-2_10.

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Schutte, W. A., L. J. Allamandola, and S. A. Sandford. "Formation of Organic Molecules by Formaldehyde Reactions in Astrophysical Ices at Very Low Temperatures." In Astrochemistry of Cosmic Phenomena. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2761-5_11.

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Samuelson, Robert. "Atmospheric Ices." In Astrophysics and Space Science Library. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5252-5_31.

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Salama, Farid. "UV Photochemistry of Ices." In Astrophysics and Space Science Library. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5252-5_11.

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9

Durham, W. B., S. H. Kirby, and L. A. Stern. "Rheology of Planetary Ices." In Astrophysics and Space Science Library. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5252-5_3.

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10

Ballering, Nicholas P., L. Ilsedore Cleeves, and Dana E. Anderson. "Simulating Protoplanetary Disk Ices." In European Conference on Laboratory Astrophysics ECLA2020. Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-29003-9_29.

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Atti di convegni sul tema "Astrophysical ices"

1

Gavdush, A. A., F. Kruczkiewicz, B. M. Giuliano, et al. "THZ-IR DIELECTRIC SPECTROSCOPY OF ASTROPHYSICAL ICES: RECENT ACHIEVEMENTS AND CHALLENGES." In Terahertz and Microwave Radiation: Generation, Detection and Applications (ТЕRА-2023). Our Style, 2023. http://dx.doi.org/10.59043/9785604953914_106.

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2

Woon, David E. "Ab Initio Quantum Chemical Studies of Reactions in Astrophysical Ices — Reactions Involving CH3OH, CO2, CO, and HNCO in H2CO/NH3/H2O Ices." In ASTROCHEMISTRY: From Laboratory Studies to Astronomical Observations. AIP, 2006. http://dx.doi.org/10.1063/1.2359569.

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3

Gargouri, Yosra, Herve Petit, Patrick Loumeau, Baptiste Cecconi, and Patricia Desgreys. "Compressed sensing for astrophysical signals." In 2016 IEEE International Conference on Electronics, Circuits and Systems (ICECS). IEEE, 2016. http://dx.doi.org/10.1109/icecs.2016.7841195.

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4

Antonov, I. O. "Experimental Capabilities of The Laboratory Apparatus for Simulation of Solid-state Astrochemical Reactions." In 52-st All-Russian with international participation student scientific conference "Physics of Space". Ural University Press, 2025. https://doi.org/10.15826/b978-5-7996-3986-0.01.

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Abstract (sommario):
Formation of complex organic molecules (COM) in the interstellar medium is a fundamental scientific problem, the solution of which requires an integrated interdisciplinary approach based on a combination of laboratory experiments, theoretical calculations of the electronic structure, modeling of conditions and processes of the interstellar medium, and astronomical observations. A unique new generation scientific apparatus for the study of cryogenic surface processes (CSP) in the interstellar medium has been built at the Center for Laboratory Astrophysics (CLA) of the Samara Branch of Lebedev P
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