EXCITED OH 4.7-GHZ MASERS ASSOCIATED WITH IRAS FAR-INFRARED SOURCES .2.

被引:40
作者
COHEN, RJ
MASHEDER, MRW
CASWELL, JL
机构
[1] UNIV BRISTOL,DEPT PHYS,BRISTOL BS8 1TL,AVON,ENGLAND
[2] AUSTRALIA TELESCOPE NATL FACIL,EPPING,NSW 2121,AUSTRALIA
关键词
MASERS; STARS; FORMATION; ISM; MOLECULES; INFRARED; LINES AND BANDS; RADIO LINES;
D O I
10.1093/mnras/274.3.808
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A sample of 85 far-infrared sources selected from the IRAS Point Source Catalog has been searched for maser emission from excited OH in the (2) Pi(1/2) J = 1/2 state, in the three transitions at 4765, 4750 and 4660 MHz. Four new detections were made at 4765 MHz, including one source where ground-state OH maser emission has not been reported. One new detection was made at 4660 MHz. This source OH 351.78 - 0.54 is remarkable in that it was detected only at 4660 MHz, and not at 4765 or 4750 MHz. Positions were measured for the new detections and for six previously known 4.7-GHz maser sources. In some cases the excited OH 4.7-GHz positions are significantly different from the positions of previously known ground-state OH 18-cm masers. The 4.7-GHz sources are among the brighter far-infrared sources in the IRAS sample. In most cases they are also OH 18-cm masers. There is a strong association between OH 4.7-GHz emission and OH 18-cm maser emission in the 1720-MHz transition. More than half of the 4.7-GHz masers that were examined for variability showed strong variations on a time-scale of a year.
引用
收藏
页码:808 / 820
页数:13
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