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Article overview
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Towards a population of HMXB/NS microquasars as counterparts of low-latitude unidentified EGRET sources | M. Ribo
; J. A. Combi
; I. F. Mirabel
; | Date: |
2 Aug 2004 | Journal: | Astrophys.Space Sci. 297 (2005) 143-154 | Subject: | astro-ph | Affiliation: | 2,3), I. F. Mirabel (1,4) ( CEA Saclay, Universidad de Jaen, Instituto Argentino de Radioastronomia, IAFE-CONICET | Abstract: | The discovery of the microquasar LS 5039 well within the 95% conficence contour of the Unidentified EGRET Source (UES) 3EG J1824-1514 was a major step towards the possible association between microquasars (MQs) and UESs. The recent discovery of precessing relativistic radio jets in LS I +61 303, a source associated for long time with 2CG 135+01 and with the UES 3EG J0241+6103, has given further support to this idea. Finally, the very recently proposed association between the microquasar candidate AX J1639.0-4642 and the UES 3EG J1639-4702 points towards a population of High Mass X-ray Binary (HMXB)/Neutron Star (NS) microquasars as counterparts of low-latitude unidentified EGRET sources. | Source: | arXiv, astro-ph/0408030 | Services: | Forum | Review | PDF | Favorites |
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