Monitoring the Gamma-Ray Source 2CG 135+1 and the Radio Star LSI+61 303

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dc.creatorTavani, M.
dc.creatorHermsen, W.
dc.creatorvan Dijk, R.
dc.creatorStrickman, M.
dc.creatorZhang, S. N.
dc.creatorFoster, R. S.
dc.creatorRay, P. S.
dc.creatorMattox, J. R.
dc.creatorUlmer, M.
dc.creatorPurcell, W.
dc.creatorCoe, M.
dc.date1996-11-25
dc.date.accessioned2026-07-07T02:22:22Z
dc.date.available2026-07-07T02:22:22Z
dc.descriptionWe report the results of a CGRO multi-instrument series of observations of the unidentified gamma-ray source 2CG 135+1 and of its possible counterpart, the peculiar radio source GT 0236+610 coincident with the Be star LSI+61 303. We monitored the time variable radio source GT 0236+610 during the CGRO observations. OSSE and COMPTEL data were obtained during the period May-June 1994, and BATSE data for the period April 1994-January 1995. We discuss the time variability of the gamma-ray emission and spectral properties of 2CG~135+1. Understanding the nature of 2CG 135+1 may be of crucial importance for the interpretation of a class of unidentified time variable gamma-ray sources in the Galaxy.
dc.description6 pages, to appear in Astronomy & Astrophys. Suppl
dc.identifierhttps://arxiv.org/abs/astro-ph/9611200
dc.identifierhttp://arxiv.org/abs/astro-ph/9611200
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10852
dc.subjectAstrophysics
dc.titleMonitoring the Gamma-Ray Source 2CG 135+1 and the Radio Star LSI+61 303
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