COMPTEL detection of the high-energy gamma-ray source 2CG 135+01
| dc.creator | van Dijk, R. | |
| dc.creator | Bennett, K. | |
| dc.creator | Bloemen, H. | |
| dc.creator | Collmar, W. | |
| dc.creator | Connors, A. | |
| dc.creator | Diehl, R. | |
| dc.creator | Hermsen, W. | |
| dc.creator | Lichti, G. G. | |
| dc.creator | McConnell, M. | |
| dc.creator | Much, R. | |
| dc.creator | Schoenfelder, V. | |
| dc.creator | Steinle, H. | |
| dc.creator | Strong, A. | |
| dc.creator | Tavani, M. | |
| dc.date | 1996-04-23 | |
| dc.date.accessioned | 2026-07-25T12:48:11Z | |
| dc.description | We present an analysis of COMPTEL observations made between November 1991 and May 1994 of 2CG 135+01, a bright gamma-ray source located near the Galactic plane. At energies above 1 MeV, an excess consistent with the position of 2CG 135+01 is detected in the sum of the observations, at flux levels which are a factor of 10-100 below those published in the past. The detection significance of this excess, when the possible presence of underlying Galactic diffuse emission is neglected, is 6.6 sigma for 3 degrees of freedom. The differential photon spectrum in the 1-30 MeV energy range can be described by a power law with a spectral index of $1.95^{+0.2}_{-0.3}$. Due to the uncertainties involved in modelling the Galactic-disk diffuse emission underneath the source, the absolute flux levels must be considered uncertain by a factor of two. They are consistent with the extrapolation of the time-averaged spectrum of 2CG 135+01 measured with EGRET, thereby strengthening the identification. No significant temporal correlation between the gamma-ray emission and the monitored radio emission of the possible counterpart radio source GT 0236+610 (showing a 26.5 day modulation) is found. | |
| dc.description | 9 pages, uses l-aa.sty, five postscript figures included. Also obtainable as postscript file at ftp://estsa2.estec.esa.nl/pub/sciproj/rvdijk_etal_AaA_23_04_96.ps.gz Accepted for publication in A&A | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9604136 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9604136 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/11923 | |
| dc.subject | Astrophysics | |
| dc.title | COMPTEL detection of the high-energy gamma-ray source 2CG 135+01 | |
| dc.type | text |