Interferometric observations of warm deuterated methanol in the inner regions of low- mass protostars Taquet, V; Bianchi, E.; Codella, C.; Persson, M., V; Ceccarelli, C.; Cabrit, S.; Jorgensen, J. K.; Kahane, C.; Lopez-Sepulcre, A.; Neri, R. Published in: Astronomy & Astrophysics DOI: 10.1051/0004-6361/201936044 Publication date: 2019 Document version Publisher's PDF, also known as Version of record Document license: CC BY-NC Citation for published version (APA): Taquet, V., Bianchi, E., Codella, C., Persson, M. V., Ceccarelli, C., Cabrit, S., Jorgensen, J. K., Kahane, C., Lopez-Sepulcre, A., & Neri, R. (2019). Interferometric observations of warm deuterated methanol in the inner regions of low-mass protostars. Astronomy & Astrophysics, 632, [A19]. https://doi.org/10.1051/0004- 6361/201936044 Download date: 02. Oct. 2021 A&A 632, A19 (2019) https://doi.org/10.1051/0004-6361/201936044 Astronomy & © ESO 2019 Astrophysics Interferometric observations of warm deuterated methanol in the inner regions of low-mass protostars? V. Taquet1, E. Bianchi2,1, C. Codella1,2, M. V. Persson3, C. Ceccarelli2, S. Cabrit4, J. K. Jørgensen5, C. Kahane2, A. López-Sepulcre2,6, and R. Neri6 1 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy e-mail:
[email protected] 2 IPAG, Université Grenoble Alpes, CNRS, 38000 Grenoble, France 3 Department of Space, Earth, and Environment, Chalmers University of Technology, Onsala Space Observatory, 439 92 Onsala, Sweden 4 LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Université, UPMC Université Paris 06, 75014 Paris, France 5 Niels Bohr Institute, University of Copenhagen, Øster Voldgade 5–7, 1350 Copenhagen K., Denmark 6 Institut de Radioastronomie Millimétrique, 38406 Saint-Martin d’Hères, France Received 7 June 2019 / Accepted 19 September 2019 ABSTRACT Methanol is a key species in astrochemistry because it is the most abundant organic molecule in the interstellar medium and is thought to be the mother molecule of many complex organic species.