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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  

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