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Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 502 (3), pp.4064-4073. ⟨10.1093/mnras/stab217⟩
Monthly Notices of the Royal Astronomical Society, 2021, 502 (3), pp.4064-4073. ⟨10.1093/mnras/stab217⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 502 (3), pp.4064-4073. ⟨10.1093/mnras/stab217⟩
Monthly Notices of the Royal Astronomical Society, 2021, 502 (3), pp.4064-4073. ⟨10.1093/mnras/stab217⟩
The analysis of the organic matter of meteorites made it possible to identify over 70 amino acids (AA), including 8 of those found in living organisms. However, their relative abundances vary drastically with the type of the carbonaceous chondrite, e
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 639, pp.A16. ⟨10.1051/0004-6361/202037839⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A16. ⟨10.1051/0004-6361/202037839⟩
Astronomy and Astrophysics-A&A, 2020, 639, pp.A16. ⟨10.1051/0004-6361/202037839⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A16. ⟨10.1051/0004-6361/202037839⟩
Context. Most of the compounds detected in the interstellar medium (ISM) that possess isomers correspond to the thermodynamically most stable isomer of a given chemical formula. Using the minimun energy principle (MEP) as a pragmatic tool is particul
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc65488e458e71dd8bece927efc6d5ab
https://hal.science/hal-02903869
https://hal.science/hal-02903869
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A125. ⟨10.1051/0004-6361/202037771⟩
UVaDOC. Repositorio Documental de la Universidad de Valladolid
instname
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A125. ⟨10.1051/0004-6361/202037771⟩
UVaDOC. Repositorio Documental de la Universidad de Valladolid
instname
Producción Científica
Context. Although H2O is the most important molecular material found in the solid state in the interstellar medium, the chemical routes leading to ice through surface reactions are still a matter of discussion. Three reac
Context. Although H2O is the most important molecular material found in the solid state in the interstellar medium, the chemical routes leading to ice through surface reactions are still a matter of discussion. Three reac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e86861be6575ff450641d09566d1c8fb
https://hal.archives-ouvertes.fr/hal-02903845/document
https://hal.archives-ouvertes.fr/hal-02903845/document
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, pp.A49. ⟨10.1051/0004-6361/201936901⟩
Astronomy and Astrophysics-A&A, 2020, 633, pp.A49. ⟨10.1051/0004-6361/201936901⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, pp.A49. ⟨10.1051/0004-6361/201936901⟩
Astronomy and Astrophysics-A&A, 2020, 633, pp.A49. ⟨10.1051/0004-6361/201936901⟩
Context. All but one complex organic molecule (COM) detected so far in the interstellar medium (ISM) are achiral; propylene oxide (c-C2H3O)-CH3 is the only exception to this. Finding other chiral species is a priority for astrobiology to progress in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab308f3ef05d94fc378d06673afe2689
https://hal.sorbonne-universite.fr/hal-02446060/document
https://hal.sorbonne-universite.fr/hal-02446060/document
Autor:
S. Baouche, François Dulieu, Isabelle Fourré, Jean-Claude Guillemin, T. Nguyen, E. Congiu, Y. Ellinger, Cécile Favre, C. Barois
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2019, 628, pp.A15. ⟨10.1051/0004-6361/201935127⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 628, pp.A15. ⟨10.1051/0004-6361/201935127⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2019, 628, pp.A15. ⟨10.1051/0004-6361/201935127⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 628, pp.A15. ⟨10.1051/0004-6361/201935127⟩
Astronomy & Astrophysics
Context. Beyond NH3, only one primary alkylamine, CH3NH2, has been identified in the interstellar medium and the reason why is still not understood: its formation could occur in the gas phase or in icy environments. Aims. To consider any possible dif
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46e36b2589822eef689ec42169e1914e
https://univ-rennes.hal.science/hal-02278393/document
https://univ-rennes.hal.science/hal-02278393/document
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 646, pp.A163. ⟨10.1051/0004-6361/202039105⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 646, pp.A163. ⟨10.1051/0004-6361/202039105⟩
Context. In spite of the permanent damage suffered from the radiation field (cosmic rays, X-rays, and intense UV-visible radiations), interstellar grains are still covered by ices mantles whose role in interstellar chemistry is well beyond any doubt.
Autor:
Jonathan I. Lunine, Stephen A. Fuselier, Ozge Ozgurel, Y. Ellinger, Kathleen Mandt, F. Pauzat, Ujjwal Raut, B. Brugger, Olivier Mousis, Thomas Ronnet, Alexis Bouquet, Romain Maggiolo, Adrienn Luspay-Kuti
Publikováno v:
Space Science Reviews
Space Science Reviews, 2018, 214, ⟨10.1007/s11214-018-0541-2⟩
Space Science Reviews, 2018, 214, ⟨10.1007/s11214-018-0541-2⟩
International audience; The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) instrument onboard the Rosetta spacecraft has measured molecular oxygen (O2) in the coma of comet 67P/Churyumov-Gerasimenko (67P/C-G) in surprisingly high
Autor:
Ozge Ozgurel, Y. Ellinger, Olivier Mousis, Steven D. Vance, François Leblanc, F. Pauzat, Alexis Markovits
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 865, pp.L16. ⟨10.3847/2041-8213/aae091⟩
The Astrophysical journal letters, 2018, 865, pp.L16. ⟨10.3847/2041-8213/aae091⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 865, pp.L16. ⟨10.3847/2041-8213/aae091⟩
The Astrophysical journal letters, 2018, 865, pp.L16. ⟨10.3847/2041-8213/aae091⟩
International audience; Sodium and potassium are known to be present as neutral elements in the exosphere of Europa. The question of the origin of these alkalis—endogenous or exogenous—remains open. They have been ascribed to exogenous contaminat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8aef5e1e8528f418e5e67ef2bd01e8ab
https://hal-insu.archives-ouvertes.fr/insu-01883891
https://hal-insu.archives-ouvertes.fr/insu-01883891
Autor:
Thomas Ronnet, Peter Wurz, K. E. Mandt, L. Le Sergeant d’Hendecourt, F. Pauzat, Jonathan I. Lunine, Pierre Vernazza, Y. Ellinger, Grégoire Danger, O. Mousis, Adrienn Luspay-Kuti
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 865 (1), pp.L11. ⟨10.3847/2041-8213/aadf89⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, ⟨10.3847/2041-8213/aadf89⟩
Mousis, O.; Ronnet, T.; Lunine, J. I.; Luspay-Kuti, A.; Mandt, K. E.; Danger, G.; Pauzat, F.; Ellinger, Y.; Wurz, P.; Vernazza, P.; Sergeant d’Hendecourt, L. Le (2018). Noble Gas Abundance Ratios Indicate the Agglomeration of 67P/Churyumov–Gerasimenko from Warmed-up Ice. Astrophysical Journal Letters, 865(1), L11. Institute of Physics Publishing IOP 10.3847/2041-8213/aadf89
The Astrophysical journal letters, 2018, ⟨10.3847/2041-8213/aadf89⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 865 (1), pp.L11. ⟨10.3847/2041-8213/aadf89⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, ⟨10.3847/2041-8213/aadf89⟩
Mousis, O.; Ronnet, T.; Lunine, J. I.; Luspay-Kuti, A.; Mandt, K. E.; Danger, G.; Pauzat, F.; Ellinger, Y.; Wurz, P.; Vernazza, P.; Sergeant d’Hendecourt, L. Le (2018). Noble Gas Abundance Ratios Indicate the Agglomeration of 67P/Churyumov–Gerasimenko from Warmed-up Ice. Astrophysical Journal Letters, 865(1), L11. Institute of Physics Publishing IOP 10.3847/2041-8213/aadf89
The Astrophysical journal letters, 2018, ⟨10.3847/2041-8213/aadf89⟩
International audience; The origin of cometary volatiles remains a major open question in planetary science. Comets may have either agglomerated from crystalline ices condensed in the protosolar nebula (PSN) or from amorphous ice originating from the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f64516c2ecd443b090abf36c8714f12b
https://hal.archives-ouvertes.fr/hal-03330174
https://hal.archives-ouvertes.fr/hal-03330174