Zobrazeno 1 - 2
of 2
pro vyhledávání: '"N. M. Murillo"'
Autor:
C. Vastel, F. Alves, C. Ceccarelli, M. Bouvier, I. Jiménez-Serra, T. Sakai, P. Caselli, L. Evans, F. Fontani, R. Le Gal, C. J. Chandler, B. Svoboda, L. Maud, C. Codella, N. Sakai, A. Lόpez-Sepulcre, G. Moellenbrock, Y. Aikawa, N. Balucani, E. Bianchi, G. Busquet, E. Caux, S. Charnley, N. Cuello, M. De Simone, F. Dulieu, A. Durân, D. Fedele, S. Feng, L. Francis, T. Hama, T. Hanawa, E. Herbst, T. Hirota, M. Imai, A. Isella, D. Johnstone, B. Lefloch, L. Loinard, M. Maureira, N. M. Murillo, S. Mercimek, S. Mori, F. Menard, A. Miotello, R. Nakatani, H. Nomura, Y. Oba, S. Ohashi, Y. Okoda, J. Ospina-Zamudio, Y. Oya, J. E. Pineda, L. Podio, A. Rimola, D. Segura Cox, Y. Shirley, L. Testi, S. Viti, N. Watanabe, Y. Watanabe, A. Witzel, C. Xue, Y. Zhang, B. Zhao, S. Yamamoto
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 664 (1), pp.171. ⟨10.1051/0004-6361/202243414⟩
Astronomy & Astrophysics, 664:A171
Astronomy and Astrophysics-A&A, 2022, 664 (1), pp.171. ⟨10.1051/0004-6361/202243414⟩
Astronomy & Astrophysics, 664:A171
C. Vastel et al.
[Aims] Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the build-up of chemical complexity in star forming regions. Thus, understanding how its abundanc
[Aims] Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the build-up of chemical complexity in star forming regions. Thus, understanding how its abundanc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e8ca2608cb4103b7f1a99218f4fa716
https://hdl.handle.net/1887/3514992
https://hdl.handle.net/1887/3514992
Autor:
Lars E. Kristensen, E. A. Bergin, R. Visser, Joseph C. Mottram, Alyssa Ramos, Luke T. Maud, Arthur D. Bosman, Jes K. Jørgensen, Michiel R. Hogerheijde, D. Harsono, Magnus Persson, N. M. Murillo, E. F. van Dishoeck
Publikováno v:
Astronomy & Astrophysics, 636, A26
Astronomy & Astrophysics
Harsono, D, Persson, M V, Ramos, A, Murillo, N M, Maud, L T, Hogerheijde, M R, Bosman, A D, Kristensen, L E, Jorgensen, J K, Bergin, E A, Visser, R, Mottram, J C & van Dishoeck, E F 2020, ' Missing water in Class I protostellar disks ', Astronomy & Astrophysics, vol. 636, A26 . https://doi.org/10.1051/0004-6361/201935994
Astronomy & Astrophysics, 636:A26. EDP Sciences
Astronomy & Astrophysics
Harsono, D, Persson, M V, Ramos, A, Murillo, N M, Maud, L T, Hogerheijde, M R, Bosman, A D, Kristensen, L E, Jorgensen, J K, Bergin, E A, Visser, R, Mottram, J C & van Dishoeck, E F 2020, ' Missing water in Class I protostellar disks ', Astronomy & Astrophysics, vol. 636, A26 . https://doi.org/10.1051/0004-6361/201935994
Astronomy & Astrophysics, 636:A26. EDP Sciences
Water is a key volatile that provides insights into the initial stages of planet formation. The low water abundances inferred from water observations toward low-mass protostellar objects may point to a rapid locking of water as ice by large dust grai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1332b0c4a9b1d21546d5629f083cd0e4
http://arxiv.org/abs/2002.11897
http://arxiv.org/abs/2002.11897