A multiwavelength investigation of the relationship between 2CG 135+1 and LSI+61°303

被引:34
作者
Strickman, MS [1 ]
Tavani, M
Coe, MJ
Steele, IA
Fabregat, J
Marti, J
Paredes, JM
Ray, PS
机构
[1] USN, Res Lab, Washington, DC 20375 USA
[2] Columbia Univ, Astrophys Lab, New York, NY 10027 USA
[3] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England
[4] Liverpool John Moores Univ, Astrophys Grp, Liverpool L3 3AF, Merseyside, England
[5] Univ Valencia, Dept Astron, E-46100 Burjassot, Spain
[6] Ctr Etud Saclay, CEA, DSM, DAPNIA,Serv Astrophys, F-91191 Gif Sur Yvette, France
[7] Univ Barcelona, Dept Astron & Meteorol, E-08028 Barcelona, Spain
关键词
binaries; close; gamma rays; observations; stars; emission-line; Be; individual; (LSI+61; degrees; 303); X-rays;
D O I
10.1086/305446
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of a multiwavelength monitoring campaign targeting the gamma-ray source 2CG 135+1 in an attempt to confirm the association of this object with the radio/Be/X-ray binary system LSI +61 degrees 303. The campaign included simultaneous radio, optical, infrared, and hard X-ray/gamma-ray observations carried out with a variety of instruments, covering (not continuously) almost three binary cycles of LSI +61 degrees 303 during the period 1994 April-July. Three separate OSSE observations of the gamma-ray source were carried out, covering different phases of the radio light curve. Hard X-ray/gamma-ray emission was detected from the direction of 2CG 135 + 1 during the first of these OSSE observations. The signal-to-noise ratio of the OSSE observations was insufficient to establish a spectral or intensity correlation of the high-energy emission with simultaneous radio, optical, and infrared emission of LSI +61 degrees 303. We briefly discuss the theoretical implications of our observations.
引用
收藏
页码:419 / 430
页数:12
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