Issue |
EAS Publications Series
Volume 75-76, 2015
Conditions and Impact of Star Formation
|
|
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Page(s) | 287 - 288 | |
Section | Star Formation Resolved: High Mass, Low Mass, and Planetary Systems | |
DOI | https://doi.org/10.1051/eas/1575058 | |
Published online | 20 May 2016 |
R. Simon, R. Schaaf and J. Stutzki (eds)
EAS Publications Series, 75–76 (2015) 287-288
Tracing the disk, envelope and outflow cavity of VLA1623 with ALMA
1 Max-Planck-Institute for extraterrestrial physics, Garching, Germany
2 Leiden Observatory, Leiden University, The Netherlands
3 Center for Astronomy, University of Heidelberg, Heidelberg, Germany
4 Institute of Astronomy and Department of Physics, National Tsing Hua University, Taiwan
5 Academia Sinica Institute of Astronomy and Astrophysics, Taiwan
Our ALMA Cycle 0 and 2 observations in Band 6 provide tracers of the disk (C18O, 13CO), the envelope (13CO, DCO+) and the outflow and its cavity (12CO, 13CO, c-C3H2) towards VLA1623, a triple non-coeval system in ρ Ophiuchus (d∼120 pc). The observations are combined with simple chemical and physical models. We find differing circumstellar envelope and outflows. VLA1623 appears to not be as chemically rich as other deeply embedded sources.
© EAS, EDP Sciences, 2016