Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-25T16:02:45.743Z Has data issue: false hasContentIssue false

Identification of Class I Methanol Masers with Objects of Near and Mid-Infrared Bands and the Third Version of the Class I Methanol Maser (MMI) Catalog

Published online by Cambridge University Press:  24 July 2012

Olga Bayandina
Affiliation:
Astro Space Center of the Lebedev Physical Institute, Moscow, Russia email: [email protected]
Irina Val'tts
Affiliation:
Astro Space Center of the Lebedev Physical Institute, Moscow, Russia email: [email protected]
Grigorii Larionov
Affiliation:
Astro Space Center of the Lebedev Physical Institute, Moscow, Russia email: [email protected]
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.

An identification has been conducted of class I methanol masers with 1) short-wave infrared objects EGO (extended green objects) - tracer bipolar outflow of matter in young stellar objects, and 2) isolated pre-protostellar gas-dust cores of the interstellar medium which are observed in absorption in the mid-infrared in the Galactic plane. It is shown that more than 50% of class I methanol masers are identified with bipolar outflows, considering the EGO as bipolar outflows (as compared with the result of 22% in the first version of the MMI catalog that contains no information about EGO). 99 from 139 class I methanol masers (71%) are identified with SDC. Thus, it seems possible that the MMI can be formed in isolated self-gravitating condensations, which are the silhouette of dark clouds - IRDC and SDC.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

Chen, X., Ellingsen, S. P., Shen, Z-Q., Titmarsh, A. et al. 2011, ApJSS, 196, Issue 1, article id.9CrossRefGoogle Scholar
Cyganowski, C. J., Whitney, B. A., Holden, E., Braden, E. et al. 2008, Astron. J., 136, 2391CrossRefGoogle Scholar
Deguchi, S., Tafoya, D., Shino, N. et al. 2011, arXiv1109.0677DGoogle Scholar
Peretto, N. & Fuller, G. A. 2009, A&A 505, 405Google Scholar
Simon, R., Jackson, J. M., Rathborne, J. M., Chambers, E. T. et al. 2006, ApJ, 639, 227CrossRefGoogle Scholar