IRAS 16293-2422 ALMA maps Virtual Observatory Resource

Authors

1. Pineda J.E.
2. Maury A.J.
3. Fuller G.A.
4. Testi L.
5. Garcia-Appadoo D.,Peck A.B.
6. Villard E.
7. Corder S.A.
8. van Kempen T.A.
9. Turner J.L.,Tachihara K.
10. Dent W.

Published by

CDS

Abstract

We focus on the kinematical properties of a proto-binary to study the infall and rotation of gas toward its two protostellar components. We present ALMA Science Verification observations with high-spectral resolution of IRAS 16293-2422 at 220.2GHz. The wealth of molecular lines in this source and the very high spectral resolution offered by ALMA allow us to study the gas kinematics with unprecedented detail.

Keywords

1. radio-sources
2. molecular-clouds
3. radio-astronomy
4. radio-continuum-emission
5. protostars

Bibliographic source Bibcode

2012A&A...544L...7P

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/544/L7

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/544/L7

Document Object Identifer DOI

doi:10.26093/cds/vizier.35449007

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/544/L7
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http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/544/L7

IVOA Table Access TAP

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IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
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