Zobrazeno 1 - 10
of 109
pro vyhledávání: '"D Despois"'
Autor:
N. Brouillet, D. Despois, J. Molet, T. Nony, F. Motte, A. Gusdorf, F. Louvet, S. Bontemps, F. Herpin, M. Bonfand, T. Csengeri, A. Ginsburg, N. Cunningham, R. Galván-Madrid, L. Maud, G. Busquet, L. Bronfman, M. Fernández-López, D. L. Jeff, B. Lefloch, Y. Pouteau, P. Sanhueza, A. M. Stutz, M. Valeille-Manet
Publikováno v:
A&A
[Context] Hot cores are signposts of the protostellar activity of dense cores in star-forming regions. W43-MM1 is a young region that is very rich in terms of high-mass star formation, which is highlighted by the presence of large numbers of high-mas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d5566c152eb3f6c7d41f4e2f9ad0382
Autor:
F. Louvet, Antoine Gusdorf, J. Molet, D. Despois, Frédérique Motte, T. Nony, N. Brouillet, Fabrice Herpin, Sylvain Bontemps
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 626, pp.A132. ⟨10.1051/0004-6361/201935497⟩
Astronomy and Astrophysics-A&A, 2019, 626, pp.A132. ⟨10.1051/0004-6361/201935497⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 626, pp.A132. ⟨10.1051/0004-6361/201935497⟩
Astronomy and Astrophysics-A&A, 2019, 626, pp.A132. ⟨10.1051/0004-6361/201935497⟩
High-mass analogues of low-mass prestellar cores are searched for to constrain the models of high-mass star formation. Several high-mass cores, at various evolutionary stages, have been recently identified towards the massive star-forming region W43-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::62e3f3acebd1b3e383d5ca950cf0e7a9
http://arxiv.org/abs/1905.12463
http://arxiv.org/abs/1905.12463
Autor:
Ana Duarte-Cabral, Q. Nguyen Luong, Kenneth A. Marsh, Timea Csengeri, Antoine Gusdorf, Edwige Chapillon, N. Brouillet, Sylvain Bontemps, J. Molet, Frédérique Motte, Anaëlle Maury, F. Louvet, D. Despois, T. Nony
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 618, pp.id.L5. ⟨10.1051/0004-6361/201833863⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 618, pp.L5. ⟨10.1051/0004-6361/201833863⟩
Astronomy and Astrophysics-A&A, 2018, 618, pp.L5. ⟨10.1051/0004-6361/201833863⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 618, pp.id.L5. ⟨10.1051/0004-6361/201833863⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 618, pp.L5. ⟨10.1051/0004-6361/201833863⟩
Astronomy and Astrophysics-A&A, 2018, 618, pp.L5. ⟨10.1051/0004-6361/201833863⟩
Aims. To constrain the physical processes that lead to the birth of high-mass stars it is mandatory to study the very first stages of their formation. We search for high-mass analogs of low-mass prestellar cores in W43-MM1. Methods. We conducted a 1.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::965455cc9da0ab031761b9e90a5b31db
https://hal.archives-ouvertes.fr/hal-01901642
https://hal.archives-ouvertes.fr/hal-01901642
Publikováno v:
Physical Chemistry Chemical Physics
Physical Chemistry Chemical Physics, 2018, 20 (8), pp.5509-5516. ⟨10.1039/C7CP05932A⟩
Physical Chemistry Chemical Physics, Royal Society of Chemistry, 2018, 20 (8), pp.5509-5516. ⟨10.1039/C7CP05932A⟩
Physical Chemistry Chemical Physics, 2018, 20 (8), pp.5509-5516. ⟨10.1039/C7CP05932A⟩
Physical Chemistry Chemical Physics, Royal Society of Chemistry, 2018, 20 (8), pp.5509-5516. ⟨10.1039/C7CP05932A⟩
International audience; Methoxymethanol, CHOCHOH is a very interesting candidate for detection in the interstellar medium since it can be formed in the recombination reaction between two radicals considered as intermediates in methanol formation: CHO
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::180fa5c8f64b7e56f822ba1da37efc80
https://hal.science/hal-01730207/document
https://hal.science/hal-01730207/document
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 620, pp.L6. ⟨10.1051/0004-6361/201834417⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 620, pp.L6. ⟨10.1051/0004-6361/201834417⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
12 pags., 3 apps.
We investigate the chemical segregation of complex O-bearing species (including the largest and most complex ones detected to date in space) towards Orion KL, the closest high-mass star-forming region. The molecular line images
We investigate the chemical segregation of complex O-bearing species (including the largest and most complex ones detected to date in space) towards Orion KL, the closest high-mass star-forming region. The molecular line images
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f9cd12b3bd4e66fcfac723f5735d8141
https://hal.archives-ouvertes.fr/hal-01934754/file/aa34417-18.pdf
https://hal.archives-ouvertes.fr/hal-01934754/file/aa34417-18.pdf
Autor:
M. Rapaport, J. F. Le Campion, Sylvain Bontemps, Hervé Bouy, Phillip A. B. Galli, Jean-Charles Cuillandre, D. Despois, Ramachrisna Teixeira, C. Ducourant, Alberto Krone-Martins
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 597, pp.A90. ⟨10.1051/0004-6361/201527574⟩
Astronomy and Astrophysics-A&A, 2017, 597, pp.A90. ⟨10.1051/0004-6361/201527574⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 597, pp.id.A90. ⟨10.1051/0004-6361/201527574⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 597, pp.A90. ⟨10.1051/0004-6361/201527574⟩
Astronomy and Astrophysics-A&A, 2017, 597, pp.A90. ⟨10.1051/0004-6361/201527574⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 597, pp.id.A90. ⟨10.1051/0004-6361/201527574⟩
We aim at performing a kinematic census of young stellar objects (YSOs) in the Rho Ophiuchi F core and partially in the E core of the L1688 dark cloud. We run a proper motion program at the ESO New Technology Telescope (NTT) with the Son of ISAAC (SO
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a923012a01a156c1993f1e3fa7eacaaa
https://hal.archives-ouvertes.fr/hal-01369504/file/aa27574-15.pdf
https://hal.archives-ouvertes.fr/hal-01369504/file/aa27574-15.pdf
Autor:
X. H. Lu, N. Brouillet, Dominique Bockelée-Morvan, Alain Baudry, José Cernicharo, D. Despois, Nicolas Biver, Jacques Crovisier
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2015, 576, pp.id.A129. ⟨10.1051/0004-6361/201424588⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 576, pp.id.A129. ⟨10.1051/0004-6361/201424588⟩
Astronomy and Astrophysics-A&A, 2015, 576, pp.id.A129. ⟨10.1051/0004-6361/201424588⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 576, pp.id.A129. ⟨10.1051/0004-6361/201424588⟩
Comparison of their chemical compositions shows, to first order, a good agreement between the cometary and interstellar abundances. However, a complex O-bearing organic molecule, ethylene glycol (CH$_{2}$OH)$_{2}$, seems to depart from this correlati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24f8b9aee353fbb73442ead2465af913
http://hdl.handle.net/20.500.12278/96013
http://hdl.handle.net/20.500.12278/96013
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Autor:
P Ehrenfreund, W Irvine, L Becker, J Blank, J R Brucato, L Colangeli, S Derenne, D Despois, A Dutrey, H Fraaije, A Lazcano, T Owen, F Robert, an International Space Science Inst ISSI-Team
Publikováno v:
Reports on Progress in Physics. 65:1427-1487
Stellar nucleosynthesis of heavy elements such as carbon allowed the formation of organic molecules in space, which appear to be widespread in our Galaxy. The physical and chemical conditions—including density, temperature, ultraviolet (UV) radiati
Publikováno v:
Astronomy & Astrophysics. 388:985-1003
Darwin (ESA) and Terrestrial Planet Finder-TPF (NASA) are two projects of space telescopes aiming at the detection of extra-solar terrestrial planets and some of their atmospheric components. In particular, they will be sensitive to the 9.6 mb and of