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2004MNRAS.352..101C - Mon. Not. R. Astron. Soc., 352, 101-111 (2004/July-3)
New OH masers at 13 441 MHz.
CASWELL J.L.
Abstract (from CDS):
At every 13441-MHz maser site, spectral features occur as right- and left-hand circularly polarized matched pairs, with small, but mostly significant, frequency separation. This is attributed to the Zeeman effect in magnetic fields of a few mG. Some of the 13441-MHz maser sites show features at several different velocities.
All of the 13441-MHz maser features have 6035-MHz counterparts that closely correspond in velocity. At three sites, features of 13441-MHz emission rival the intensities of their 6035-MHz counterparts; at the other sites, features are weaker than at 6035 MHz by factors of between 3 and 50. Upper limits at some sites searched can be set more than 2 orders of magnitude weaker than 6035-MHz emission. The detection statistics provide unique opportunities to test recent advances in maser modelling.
A search for the 13434-MHz transition towards the same 56 targets yielded no detections.
Abstract Copyright: 2004 RAS
Journal keyword(s): masers - stars: formation - HII regions - ISM: molecules - radio lines: ISM
Simbad objects: 60
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