Detection of new sources of methanol emission at 95 GHz with the Mopra telescope

Citation
Ie. Val'Tts et al., Detection of new sources of methanol emission at 95 GHz with the Mopra telescope, M NOT R AST, 317(2), 2000, pp. 315-332
Citations number
30
Categorie Soggetti
Space Sciences
Journal title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN journal
00358711 → ACNP
Volume
317
Issue
2
Year of publication
2000
Pages
315 - 332
Database
ISI
SICI code
0035-8711(20000911)317:2<315:DONSOM>2.0.ZU;2-Q
Abstract
A southern hemisphere survey of methanol emission sources has been carried out using the Australia Telescope National Facility Mopra millimetre telesc ope. 85 sources, the majority of them masers, have been detected in the 8(0 )-7(1) A(+) transition of methanol at 95 GHz. Together with a similar north ern hemisphere survey, this completes the search for 95-GHz methanol emissi on from the Galactic plane. The previously found correlation between intens ities of methanol emission at 44 and 95 GHz is confirmed here with the larg er sample of sources. The results of large velocity gradient statistical eq uilibrium calculations confirm the classification of these sources as class I methanol masers pumped through collisional excitation.