IRAS 14070+0525 - AN OH GIGAMASER AT Z = 0.265

被引：34

作者：

BAAN, WA

RHOADS, J

FISHER, K

ALTSCHULER, DR

HASCHICK, A

机构：

[1] HARVARD UNIV,DEPT ASTRON,CAMBRIDGE,MA 02139

[2] UNIV CALIF BERKELEY,DEPT ASTRON,BERKELEY,CA 94720

[3] UNIV PUERTO RICO,DEPT PHYS,RIO PIEDRAS,PR 00631

[4] HAYSTACK OBSERV,WESTFORD,MA 01886

来源：

ASTROPHYSICAL JOURNAL | 1992年 / 396卷 / 02期

关键词：

GALAXIES; ACTIVE; INDIVIDUAL; IR; 14070+0525; INTERSTELLAR MATTER; MASERS; RADIO LINES; MOLECULAR; INTERSTELLAR;

D O I：

10.1086/186526

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

OH gigamaser emission has been detected in the luminous FIR galaxy IRAS 14070 + 0525 at a redshift of 0.265. The FIR luminosity of IRAS 14070 + 0525 is 10(12.5) L . . The OH line luminosity is 1.4 x 10(4) L . , making it the most luminous known OH emitter. The OH line emission covers a velocity range of approximately 2400 km s-1. Two distinct components in the OH emission reveal a powerful outflow component and/or the interactive nature of the system.

引用

页码：L99 / L102

页数：4

共 22 条

[1]

[Anonymous], 1988, IRAS POINT SOURCE CA

[2]

Baan W.A., 1991, ASP C SER, V16, P45

[3] INFRARED PROPERTIES OF OH GALAXIES [J].