The detection of new methanol masers in the 5(-1)-4(0)E line

Citation
Sv. Kalenskii et al., The detection of new methanol masers in the 5(-1)-4(0)E line, ASTRON REP, 45(1), 2001, pp. 26-33
Citations number
18
Categorie Soggetti
Space Sciences
Journal title
ASTRONOMY REPORTS
ISSN journal
10637729 → ACNP
Volume
45
Issue
1
Year of publication
2001
Pages
26 - 33
Database
ISI
SICI code
1063-7729(200101)45:1<26:TDONMM>2.0.ZU;2-O
Abstract
Forty-eight objects were detected in the 5(-1)(-4)0(E) methanol line at 83. 5 GHz during a survey of Class I maser sources. Narrow maser features were found in 14 of these. Broad quasi-thermal lines were detected toward other sources. One of the objects with narrow features at 84.5 GHz, the young bip olar outflow L1157, was also observed in the 8(0)-7(1)A(+) line at 95.2 GHz : a narrow line was detected at this frequency. Analysis showed that the br oad lines are usually inverted. The quasi-thermal profiles imply that there are no more than a few line opacities. These results confirm the plausibil ity of models in which compact Class I masers appear in extended sources as a result of a preferential velocity field. (C) 2001 MAIK "Nauka/Interperio dica".