Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999apj...519..244m&link_type=abstract
The Astrophysical Journal, Volume 519, Issue 1, pp. 244-256.
Astronomy and Astrophysics
Astronomy
24
Ism: H Ii Regions, Ism: Individual: Alphanumeric: W3, Ism: Molecules, Masers, Radio Lines: Ism, Stars: Formation
Scientific paper
We have conducted VLBA observations of the 12 GHz CH_3OH masers toward the ultracompact H II region W3(OH). The angular resolution of ~1 mas is sufficient to resolve most of the maser spots and determine their sizes and brightness temperatures. The FWHM sizes of the spots are found from <=2 to 10 AU with brightness temperatures between 10^9 and 6x10^11 K. The actual brightness temperatures may be higher (by a factor <=10) than the measured values, because most of the spots have spectral profiles unresolved with our velocity resolution (0.28 km s^-1). Our data also suggest the presence ofa spatially extended component of maser emission with size >=20 mas and brightness temperature<=10^9 K. The comparison of our data with previous 6.7 GHz VLBI observations shows that there is a good spatial (<=10 mas) and velocity (within 0.3 km s^-1) correspondence between numerous 12 and 6.7 GHz CH_3OH spots. Comparing our maps with those of Menten et al. yields relative proper motions of a few km s^-1 in magnitude. A ``linear structure'' of approximately 200 AU in size (P.A.=141^deg) is found in the northern methanol maser clump, which also shows a regular trend of radial velocities with projected positions (a velocity gradient of 2400 km s^-1 pc^-1).
Menten Karl. M.
Moscadelli Luca
Reid Mark J.
Walmsley Charles Malcolm
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