Co-propagation of maser emission at 1720 and 4765 MHz

Citation
Md. Gray et al., Co-propagation of maser emission at 1720 and 4765 MHz, M NOT R AST, 324(3), 2001, pp. 643-647
Citations number
17
Categorie Soggetti
Space Sciences
Journal title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN journal
00358711 → ACNP
Volume
324
Issue
3
Year of publication
2001
Pages
643 - 647
Database
ISI
SICI code
0035-8711(20010701)324:3<643:COMEA1>2.0.ZU;2-T
Abstract
MERLIN observations are presented of OH 4765-MHz and OH 1720-MHz masers in the massive star-forming region W3(OH). Two of the three intense spots of m aser emission at 4765 MHz are spatially coincident with two similar spots a t 1720 MHz in both left-hand circular (LHC) and right-hand circular (RHC) p olarizations, to an accuracy of 15 mas. The spots also overlap in velocity when allowance is made for Zeeman splitting of the 1720-MHz Line. We conclu de that we have found two examples of masers in different rotational levels of OH which are co-propagating through the same column of gas and experien cing competitive gain effects. The third 4765-MHz maser spot was found to h ave no overlapping counterpart amongst the 1720-MHz masers.