SIMBAD references

2006ApJ...638..241E - Astrophys. J., 638, 241-261 (2006/February-2)

Methanol masers: reliable tracers of the early stages of high-mass star formation.

ELLINGSEN S.P.

Abstract (from CDS):

The GLIMPSE and MSX surveys have been used to examine the mid-infrared properties of a statistically complete sample of 6.7 GHz methanol masers. The GLIMPSE point sources associated with methanol masers are clearly distinguished from the majority, typically having extremely red mid-infrared colors similar to those expected of low-mass Class 0 young stellar objects. The intensity of the GLIMPSE sources associated with methanol masers is typically 4 mag brighter at 8.0 µm than at 3.6 µm. Targeted searches toward GLIMPSE point sources with [3.6]-[4.5]>1.3 and an 8.0 µm magnitude less than 10 will detect more than 80% of Class II methanol masers. Many of the methanol masers are associated with sources within infrared dark clouds (IRDCs), which are believed to mark regions where high-mass star formation is in its very early stages. The presence of Class II methanol masers in a significant fraction of IRDC suggests that high-mass star formation is common in these regions. Different maser species are thought to trace different evolutionary phases of the high-mass star formation process. Comparison of the properties of the GLIMPSE sources associated with Class II methanol masers and other maser species shows interesting trends, consistent with Class I methanol masers tracing a generally earlier evolutionary phase and OH masers tracing a later evolutionary phase.

Abstract Copyright:

Journal keyword(s): Infrared: ISM - ISM: Molecules - Masers - Radio Lines: ISM - Stars: Formation

Simbad objects: 41

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2019.12.07-21:05:07

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