AN EXCITED-STATE OH MASER IN THE LARGE MAGELLANIC CLOUD

Authors
Citation
Jl. Caswell, AN EXCITED-STATE OH MASER IN THE LARGE MAGELLANIC CLOUD, Monthly Notices of the Royal Astronomical Society, 272(4), 1995, pp. 31-34
Citations number
16
Categorie Soggetti
Astronomy & Astrophysics
ISSN journal
00358711
Volume
272
Issue
4
Year of publication
1995
Pages
31 - 34
Database
ISI
SICI code
0035-8711(1995)272:4<31:AEOMIT>2.0.ZU;2-1
Abstract
A maser at the 6.035-GHz transition of excited OH has been discovered in the Large Magellanic Cloud. It is the first extragalactic maser fou nd at this transition, and is at the position of a previously known 1. 665-GHz ground-state maser. It is stronger in the excited state than i n the ground state, a characteristic shared by only six of the 78 simi lar excited-state OH masers detected in our Galaxy. An accurate positi on for the maser and a high-resolution continuum map have also been ob tained. These show that the maser is 50 arcsec south-west of the peak of an H II region known optically as N160a (not towards N159 as was su ggested from the ground-state maser discovery measurements); it is at the location of a 3-mJy continuum radio source, probably a weak H II r egion.