NARROW EMISSION-LINE NEAR 1720MHZ IN DIRECTION OF SGRA

被引：4

作者：

WHITEOAK, JB ^{[1
]}

GARDNER, FF ^{[1
]}

机构：

[1] CSIRO,DIV RADIOPHYS,POB 76,EPPING 2121,NEW S WALES,AUSTRALIA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1975年 / 173卷 / 01期

关键词：

D O I：

10.1093/mnras/173.1.25P

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A narrow emission feature (of half-width 4·5 km s-1 in velocity) has been detected in the 1720 MHz OH-line spectrum of Sgr A at a frequency that would correspond to an OH velocity of + 132 km s-1 (lsr). However, the identification as an OH transition is questioned because there are no features of similar velocity in the line profiles of either the other OH ground-state transitions or transitions for other molecules. © 1975 Royal Astronomical Society.

引用

页码：P25 / P28

页数：4

共 8 条

[1] Gardner F. F., 1974, Proceedings of the Astronomical Society of Australia, V2, P253
[2] KERR FJ, 1967, AUST J PHYS S3
[3] V1057 CYGNI OH SOURCE - TIME VARIATION, POLARIZATION PROPERTIES, AND ACCURATE POSITION
LO, KY
BECHIS, KP
[J]. ASTROPHYSICAL JOURNAL, 1974, 190 (03) : L125 - L128
[4] ROBINSON BJ, 1970, AUST J PHYS, V23, P363
[5] Rougoor G. W., 1964, B ASTRON I NETH, V17, P381
[6] SANDERS RH, 1974, ASTRON ASTROPHYS, V33, P9
[7] WHITEOAK JB, 1974, ASTRON ASTROPHYS, V36, P245
[8] ANOMALIES IN 18-CENTIMETER OH LINES IN GALAXY NGC 4945
WHITEOAK, JB
GARDNER, FF
[J]. ASTROPHYSICAL JOURNAL, 1975, 195 (02) : L81 - L84

← 1 →