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A&A 369, 278-290 (2001)
DOI: 10.1051/0004-6361:20010124
VLBI observations of 6.7 and 12.2 GHz methanol masers toward high mass star-forming regions
II. Tracing massive protostars
V. Minier, J. E. Conway and R. S. BoothOnsala Space Observatory, 439 92 Onsala, Sweden
(Received 20 November 2000 / Accepted 22 January 2001)
Abstract
We compare the absolute positions of methanol maser
sites with those of typical tracers of young massive stellar
objects, such as ultra-compact HII regions, outflows and hot molecular cores. We have
selected thirteen star-forming regions for which we have produced VLBI maps of 6.7 and
12.2 GHz methanol masers, and for which complementary high resolution images
are available in the literature. These sources are namely: IRAS 20126+4104,
NGC 7538, S 252, G 31.28+0.06, W 75N, S 255, S 269, Mon R2, G 9.62+0.20,
Cep A, W 51, G 59.78+0.06 and G 29.95-0.02. Eight of the methanol maser sources coincide in position
within 2000 AU with outflows and/or hot molecular cores, i.e. phenomena occuring at the earliest
stage of massive star formation. Only two sources coincide in position with
hyper-compact HII regions. We conclude that 6.7 and 12.2 GHz methanol masers are likely to be one of
the first signposts of massive star formation and perhaps the first signpost of a massive protostar.
Key words: HII regions -- masers -- stars: formation -- circumstellar matter -- techniques: interferometric
Offprint request: V. Minier, vincent@oso.chalmers.se
SIMBAD Objects
© ESO 2001
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