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pro vyhledávání: '"621"'
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2019, 621, pp.A124. ⟨10.1051/0004-6361/201833314⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 621, pp.A124. ⟨10.1051/0004-6361/201833314⟩
Astronomy and Astrophysics-A&A, 2019, 621, pp.A124. ⟨10.1051/0004-6361/201833314⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 621, pp.A124. ⟨10.1051/0004-6361/201833314⟩
With the discovery over the last two decades of a large diversity of exoplanetary systems, it is now of prime importance to characterize star-planet interactions and how such systems evolve. We address this question by studying systems formed by a so
Autor:
Alfred Vidal-Madjar, A. Lecavelier des Etangs, Paul Wilson, Ignas Snellen, Flavien Kiefer, Vincent Bourrier, R. Kerr
Publikováno v:
Astronomy & Astrophysics
Astronomy and Astrophysics (0004-6361), 621, A121
Astronomy and Astrophysics (0004-6361), 621, A121
The debris disk surrounding $\beta$ Pictoris has a gas composition rich in carbon and oxygen, relative to solar abundances. Two possible scenarios have been proposed to explain this enrichment. The preferential production scenario suggests that the g
Autor:
Stephan Schlemmer, Holger S. P. Müller, Frank Lewen, Olena Zakharenko, Vadim V. Ilyushin, Jes K. Jørgensen, Maria Drozdovskaya
Publikováno v:
Astronomy & Astrophysics
Zakharenko, O, Lewen, F, Ilyushin, V V, Drozdovskaya, M N, Jorgensen, J K, Schlemmer, S & Mueller, H S P 2019, ' Deuterated methyl mercaptan (CH3SD): Laboratory rotational spectroscopy and search toward IRAS 16293-2422 B ', Astronomy & Astrophysics, vol. 621, A114 . https://doi.org/10.1051/0004-6361/201834472
Zakharenko, O, Lewen, F, Ilyushin, V V, Drozdovskaya, M N, Jorgensen, J K, Schlemmer, S & Mueller, H S P 2019, ' Deuterated methyl mercaptan (CH3SD): Laboratory rotational spectroscopy and search toward IRAS 16293-2422 B ', Astronomy & Astrophysics, vol. 621, A114 . https://doi.org/10.1051/0004-6361/201834472
Methyl mercaptan (also known as methanethiol), CH3SH, has been found in the warm and dense parts of high -- as well as low -- mass star-forming regions. The aim of the present study is to obtain accurate spectroscopic parameters of the S-deuterated m