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Chemical Tracers of Dynamics in Low-Mass Protostellar Objects

Published online by Cambridge University Press:  04 September 2018

Satoshi Yamamoto ,
Yoko Oya Open the ORCID record for Yoko Oya [Opens in a new window]  and
Nami Sakai
Satoshi Yamamoto
Affiliation:
Department of Physics, The University of Tokyo, Bunkyo-ku, Tokyo, 113-0033, Japan email: yamamoto@taurus.phys.s.u-tokyo.ac.jp, oya@taurus.phys.s.u-tokyo.ac.jp
Yoko Oya
Affiliation:
Department of Physics, The University of Tokyo, Bunkyo-ku, Tokyo, 113-0033, Japan email: yamamoto@taurus.phys.s.u-tokyo.ac.jp, oya@taurus.phys.s.u-tokyo.ac.jp
Nami Sakai
Affiliation:
RIKEN, Wako, Saitama, 351-0198, Japan email: nami.sakai@riken.jp
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Abstract

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Recent progress in astrochemistry of low-mass protostellar sources is reviewed. In particular, we focus on disk formation processes and associated chemical changes at a 50 au scale, which is extensively being studied with ALMA. A small scale chemical differentiation sensitively reflects changes in physical conditions, and hence, it provides us with unique opportunities of chemical diagnostics of disk-forming regions. Complex physical and chemical pictures of disk formation revealed by observations are summarized, and future prospects are discussed.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S332: Astrochemistry VII: Through the Cosmos from Galaxies to Planets , March 2017 , pp. 175 - 186
Copyright
Copyright © International Astronomical Union 2018 

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