6533b828fe1ef96bd1287a73

RESEARCH PRODUCT

A Multiwavelength Investigation of the Relationship Between 2CG135+1 and LSI+61o 303

M. S. StrickmanJ. M. ParedesJuan FabregatIain A. SteeleM. J. CoeMarco TavaniPaul S. RayJosep Martí

subject

PhysicsSignal-to-noise ratioSpace and Planetary ScienceInfraredAstrophysics (astro-ph)Binary numberFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsQCQB

description

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 +61o 303. The campaign included simultaneous radio, optical, infrared, and hard x-ray/gamma-ray observations carried out with a variety of instruments, covering (not continously) almost three binary cycles of LSI +61o 303 during the period April-July 1994. Three separate OSSE observations of the gamma-ray source were carried out, covering different phases of the radio lightcurve. 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 +61o 303. We briefly discuss the theoretical implications of our observations.

https://dx.doi.org/10.48550/arxiv.astro-ph/9711286