Streamers feeding the SVS13-A protobinary system: astrochemistry reveals accretion shocks?

Author:

Bianchi Eleonora1ORCID,López-Sepulcre Ana23ORCID,Ceccarelli Cecilia2ORCID,Codella Claudio42ORCID,Podio Linda4ORCID,Bouvier Mathilde5ORCID,Enrique-Romero Joan6ORCID,Bachiller Rafael7ORCID,Lefloch Bertrand28ORCID

Affiliation:

1. Excellence Cluster ORIGINS, Boltzmannstraße 2, Garching bei München, 85748, Germany

2. Univ. Grenoble Alpes, CNRS, IPAG, 38000 Grenoble, France

3. Institut de Radioastronomie Millimétrique, 38406 Saint-Martin d' Hères, France

4. INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, Firenze, I-50125, Italy

5. Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands

6. Leiden Institute of Chemistry, Gorlaeus Laboratories, Leiden University, P.O. Box 9502, 2300 RA Leiden, The Netherlands

7. Observatorio Astronómico Nacional (OAN-IGN), Alfonso XII 3, 28014 Madrid, Spain

8. Laboratoire d'astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, Allée Geoffroy Saint-Hilaire, 33615 Pessac, France

Abstract

We analyse deuterated water (HDO) and sulfur dioxide (SO2) at high-angular resolution in the binary system SVS13-A. We propose that molecular emission is produced by an accretion shock at the interface between the accretion streamer and the disk.

Funder

Deutsche Forschungsgemeinschaft

European Commission

Publisher

Royal Society of Chemistry (RSC)

Subject

Physical and Theoretical Chemistry

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