Hostname: page-component-8448b6f56d-qsmjn Total loading time: 0 Render date: 2024-04-23T17:55:06.953Z Has data issue: false hasContentIssue false

Shocked CO and 13CO around Wolf-Rayet ring nebulae

Published online by Cambridge University Press:  26 May 2016

J. Ricardo Rizzo
Affiliation:
Departamento de Física, Universidad Europea CEES, E-28670, Villaviciosa de Odón, España Observatorio Astronómico Nacional, Aptdo. Correos 1143, E-28800 Alcalá de Henares, España
Jesús Martín-Pintado
Affiliation:
Observatorio Astronómico Nacional, Aptdo. Correos 1143, E-28800 Alcalá de Henares, España
Jean-François Desmurs
Affiliation:
Observatorio Astronómico Nacional, Aptdo. Correos 1143, E-28800 Alcalá de Henares, España

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.

We show CO and 13CO maps toward the WR nebulae NGC 2359, NGC 6888 and Anon (WR 134). We determine global parameters and discuss the probable origin of this gas. Nowadays it is becoming clear that molecule formation and survival is be possible around massive evolved stars.

Type
Part 4. Feedback from Massive Stars
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Cappa, C.E., Rubio, M., Goss, W.M. 2001, AJ 121, 2664.CrossRefGoogle Scholar
Marston, A.P., Welzmiller, J., Bransford, M.A., Black, J.H., Bergman, P. 1999, ApJ 518, 769.CrossRefGoogle Scholar
Rizzo, J.R., Martín-Pintado, J., Mangum, J.G. 2001a, A&A 366, 146.Google Scholar
Rizzo, J.R., Martín-Pintado, J., Henkel, C. 2001b, ApJ (Letters) 553, L181.CrossRefGoogle Scholar
St-Louis, N., Doyon, R., Chagnon, F., Nadeau, D. 1998, AJ 115, 2475.CrossRefGoogle Scholar