CO(2-1) maps of IRAS 00117+6412 Virtual Observatory Resource

Authors

1. Palau A.
2. Sanchez-Monge A.
3. Busquet G.
4. Estalella R.
5. Zhang Q.
6. Ho P.T.P.,Beltran M.T.
7. Beuther H.

Published by

CDS

Abstract

Our main aim is to study the influence of the initial conditions of a cloud in the intermediate/high-mass star formation process. We observed with the VLA, PdBI, and SMA the centimeter and millimeter continuum, N_2_H^+^ (1-0), and CO (2-1) emission associated with a dusty cloud harboring a nascent cluster with intermediate-mass protostars.

Keywords

1. infrared-sources
2. young-stellar-objects
3. radio-sources

Bibliographic source Bibcode

2010A&A...510A...5P

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/510/A5

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/510/A5

Document Object Identifer DOI

doi:10.26093/cds/vizier.35100005

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