|
1.
|
|
17 p, 2.9 MB |
V. Hot methanol in the [BHB2007] 11 protobinary system; Hot corino versus shock origin
/
Vastel, C. (Université de Toulouse) ;
Alves, F. (Université Grenoble Alpes) ;
Ceccarelli, Cecilia (Université Grenoble Alpes) ;
Bouvier, M. (Université Grenoble Alpes) ;
Jiménez-Serra, I. (Centro de Astrobiología (Madrid)) ;
Sakai, T. (University of Electro-Communications) ;
Caselli, P. (Max Planck Institute for Extraterrestrial Physics) ;
Evans, L. (Université de Toulouse) ;
Fontani, F. (Osservatorio Astrofisico Di Arcetri) ;
Le Gal, R. (Institute for Planetary sciences and Astrophysics) ;
Chandler, C. J. (National Radio Astronomy Observatory Socorro) ;
Svoboda, B. (National Radio Astronomy Observatory Socorro) ;
Maud, L. (ESO Supernova Planetarium & Visitor Centre) ;
Codella, Claudio (Institute for Planetary sciences and Astrophysics) ;
Sakai, N. (RIKEN) ;
López-Sepulcre, A. (Institute for Planetary sciences and Astrophysics) ;
Moellenbrock, G. (National Radio Astronomy Observatory Socorro) ;
Aikawa, Y. (The University of Tokyo) ;
Balucani, Nadia (Università degli studi di Perugia) ;
Bianchi, E. (Institute for Planetary sciences and Astrophysics) ;
Busquet, G. (Universitat de Barcelona) ;
Caux, E. (Université de Toulouse) ;
Charnley, S. (NASA Goddard Space Flight Center) ;
Cuello, N. (Institute for Planetary sciences and Astrophysics) ;
De Simone, M. (Institute for Planetary sciences and Astrophysics) ;
Dulieu, F. (CY Cergy Paris Université) ;
Durán, A. (Instituto de Radioastronomía y Astrofísica) ;
Fedele, D. (Osservatorio Astrofisico Di Arcetri) ;
Feng, S. (Xiamen University) ;
Francis, L. (University of Victoria BC) ;
Hama, T. (The University of Tokyo) ;
Hanawa, T. (Chiba University. Center for Frontier Science) ;
Herbst, E. (University of Virginia) ;
Hirota, T. (National Astronomical Observatories) ;
Imai, M. (The University of Tokyo) ;
Isella, A. (Rice University) ;
Johnstone, D. (University of Victoria BC) ;
Lefloch, B. (Institute for Planetary sciences and Astrophysics) ;
Loinard, L. (Universidad Nacional Autónoma de México. Instituto de Radioastronomía y Astrofísica) ;
Maureira, M. (Max Planck Institute for Extraterrestrial Physics) ;
Murillo, N. M. (RIKEN) ;
Mercimek, S. (Osservatorio Astrofisico Di Arcetri) ;
Mori, S. (Tohoku University) ;
Menard, F. (Institute for Planetary sciences and Astrophysics) ;
Miotello, A. (ESO Supernova Planetarium & Visitor Centre) ;
Nakatani, R. (RIKEN) ;
Nomura, H. (Chinese Academy of Sciences) ;
Oba, Y. (Hokkaido University) ;
Ohashi, S. (RIKEN) ;
Okoda, Y. (The University of Tokyo) ;
Ospina-Zamudio, J. (Institute for Planetary sciences and Astrophysics) ;
Oya, Y. (The University of Tokyo) ;
Pineda, J. E. (Max Planck Institute for Extraterrestrial Physics) ;
Podio, L. (Osservatorio Astrofisico Di Arcetri) ;
Rimola, Albert (Universitat Autònoma de Barcelona. Departament de Química) ;
Cox, D. Segura (Max Planck Institute for Extraterrestrial Physics) ;
Shirley, Y. (University of Arizona) ;
Testi, L. (Osservatorio Astrofisico Di Arcetri) ;
Viti, S. (University of Leiden) ;
Watanabe, N. (Hokkaido University) ;
Watanabe, Y. (Shibaura Institute of Technology) ;
Witzel, A. (Institute for Planetary sciences and Astrophysics) ;
Xue, C. (University of Virginia) ;
Zhang, Y. (RIKEN) ;
Zhao, B. (Max Planck Institute for Extraterrestrial Physics) ;
Yamamoto, S. (The University of Tokyo)
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 abundance evolves during the star formation process and whether it enriches the emerging planetary system is of paramount importance. [...]
2022 -  10.1051/0004-6361/202243414
Astronomy & astrophysics, Vol. 664 (August 2022) , art. A171
|
|
|
2.
|
|
11 p, 1.3 MB |
Acetaldehyde binding energies : a coupled experimental and theoretical study
/
Ferrero, Stefano (Universitat Autònoma de Barcelona. Departament de Química) ;
Grieco, F. (University of Ghent. Department of Physics and Astronomy) ;
Ibrahim Mohamed, A-S (Centre National de la Recherche Scientifique. Sorbonne Université) ;
Dulieu, François (Centre National de la Recherche Scientifique. Sorbonne Université) ;
Rimola, Albert (Universitat Autònoma de Barcelona. Departament de Química) ;
Ceccarelli, Cecilia (Centre National de la Recherche Scientifique. Université Grenoble Alpes) ;
Nervi, C. (Università degli Studi di Torino. Dipartimento di Chimica) ;
Minissale, M. (Centre National de la Recherche Scientifique. Aix-Marseille University) ;
Ugliengo, Piero (Università degli Studi di Torino. Dipartimento di Chimica)
Acetaldehyde is one of the most common and abundant gaseous interstellar complex organic molecules found in cold and hot regions of the molecular interstellar medium. Its presence in the gas-phase depends on the chemical formation and destruction routes, and its binding energy (BE) governs whether acetaldehyde remains frozen on to the interstellar dust grains or not. [...]
2022 - 10.1093/mnras/stac2358
Monthly Notices of the Royal Astronomical Society, Vol. 516, Issue 2 (October 2022) , p. 2586-2596
|
|
guest ::
email alert
or subscribe to the 
RSS feed.
