FAUST: V. Hot methanol in the [BHB2007] 11 protobinary system; hot corino versus shock origin

Author(s):
Vastel, C.; Alves, F.; Ceccarelli, C.; Bouvier, M.; Jiménez-Serra, I.; Sakai, T.; Caselli, P.; Evans, L.; Fontani, F.; Le Gal, R.; Chandler, C.J.; Svoboda, B.; Maud, L.; Codella, C.; Sakai, N.; López-Sepulcre, A.; Moellenbrock, G.; Aikawa, Y.; Balucani, N.; Bianchi, E.; Busquet, G.; Caux, E.; Charnley, S.; Cuello, N.; De Simone, M.; Dulieu, F.; Durân, A.; Fedele, D.; Feng, S.; Francis, L.; Hama, T.; Hanawa, T.; Herbst, E.; Hirota, T.; Imai, M.; Isella, A.; Johnstone, D.; Lefloch, B.; Loinard, L.; Maureira, M.; Murillo, N.M.; Mercimek, S.; Mori, S.; Menard, F.; Miotello, A.; Nakatani, R.; Nomura, H.; Oba, Y.; Ohashi, S.; Okoda, Y.; Ospina-Zamudio, J.; Oya, Y.; Pineda, J.E.; Podio, L.; Rimola, A.; Segura Cox, D.; Shirley, Y.; Testi, L.; Viti, S. (0000-0001-8504-8844); Watanabe, N.; Watanabe, Y.; Witzel, A.; Xue, C.; Zhang, Y.; Zhao, B.; Yamamoto, S.
Published
2022
Publication type
Article / Letter to editor
AstrochemistryRadiative transferInterferometric techniquesLineIdentificationAbundances and molecules (ISM)Astrophysics of galaxiesSolar and stellar astrophysics
Date issued
2022
Language
English
Is part of
Astronomy & Astrophysics (2022), A171
hdl
1887/3514992
doi
10.1051/0004-6361/202243414
URL
https://ui.adsabs.harvard.edu/abs/2022A&A...664A.171V