Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-15T05:03:53.307Z Has data issue: false hasContentIssue false
  • English
  • Français

Formaldehyde observations at XAO

Published online by Cambridge University Press:  21 March 2013

Gang Wu ,
Jarken Esimbek ,
Jian-Jun Zhou  and
Wei-Guang Ji
Gang Wu
Affiliation:
Xinjiang Astronomical Observatory, CAS Postbus 830011, 150 Science 1-Street, Urumuqi, China email: wug@xao.ac.cn
Jarken Esimbek
Affiliation:
Xinjiang Astronomical Observatory, CAS Postbus 830011, 150 Science 1-Street, Urumuqi, China email: wug@xao.ac.cn
Jian-Jun Zhou
Affiliation:
Xinjiang Astronomical Observatory, CAS Postbus 830011, 150 Science 1-Street, Urumuqi, China email: wug@xao.ac.cn
Wei-Guang Ji
Affiliation:
Xinjiang Astronomical Observatory, CAS Postbus 830011, 150 Science 1-Street, Urumuqi, China email: wug@xao.ac.cn
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In recent years our team has performed H2CO(110 − 111) observations towards GMCs and HII regions with the Xinjiang Astronomical Observatory, CAS. Here, we provide a summary of these observations. More than 200 new formaldehyde sources are detected, 8 extended GMC have been mapped, kinetic distances, Galactic structure and a related discussion are provided.

Keywords

ISM: clouds — HII regions
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 62
Copyright
Copyright © International Astronomical Union 2013

References

Townes, C. H. & Cheung, A. C., 1969, ApJ, 157, L103CrossRefGoogle Scholar