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相关论文: Unidentified gamma-ray sources off the Galactic pl…

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Population studies of EGRET gamma-ray sources indicate that there is a distinctive population of bright sources at low galactic latitudes. The sources have a distribution consistent with that of young galactic objects, with a concentration…

天体物理学 · 物理学 2009-11-10 Valenti Bosch-Ramon , Gustavo E. Romero , Josep M. Paredes

Population studies of unidentified EGRET sources suggest that there exist at least three different populations of galactic gamma-ray sources. One of these populations is formed by young objects distributed along the galactic plane with a…

天体物理学 · 物理学 2009-11-10 V. Bosch-Ramon , G. E. Romero , J. M. Paredes

The all-sky survey in high-energy gamma rays (E$>$30 MeV) carried out by the Energetic Gamma Ray Experiment Telescope (EGRET) aboard the Compton Gamma-Ray Observatory provides a unique opportunity to examine in detail the diffuse gamma-ray…

天体物理学 · 物理学 2011-05-05 P. Sreekumar

Some phenomenological properties of the unidentified EGRET detections suggest that there are two distinct groups of galactic gamma-ray sources that might be associated with compact objects endowed with relativistic jets. We discuss…

天体物理学 · 物理学 2007-05-23 G. E. Romero , I. A Grenier , M. M. Kaufman Bernado , I. F. Mirabel , D. F. Torres

The recent discovery by Paredes et al. (2000) of a persistent microquasar that is positionally coincident with an unidentified gamma-ray source has open the possibility that other sources in the Third EGRET Catalog could be interpreted as…

天体物理学 · 物理学 2009-11-07 M. M. Kaufman Bernado , G. E. Romero , I. F. Mirabel

A review of the main characteristics of low-latitude sources in the third EGRET catalog is presented. There are 75 unidentified gamma-ray sources detected by EGRET at less than 10 degrees from the galactic plane. About a half of these…

天体物理学 · 物理学 2007-05-23 Gustavo E. Romero

Microquasars, X-ray binary systems that generate relativistic jets, were discovered in our Galaxy in the last decade of the XXth century. Their name indicates that they are manifestations of the same physics as quasars but on a completely…

天体物理学 · 物理学 2009-11-11 M. M. Kaufman Bernado

Among unidentified gamma-ray sources in the galactic plane, there are some that present significant variability and have been proposed to be high-mass microquasars. To deepen the study of the possible association between variable low…

天体物理学 · 物理学 2009-11-11 V. Bosch-Ramon , J. M. Paredes , G. E. Romero , D. F. Torres

Diffuse Galactic gamma-ray emission is produced in interactions of cosmic rays with gas and ambient photon fields and thus provides us with an indirect measurement of cosmic rays in various locations in the Galaxy. The diffuse gamma-ray…

天体物理学 · 物理学 2007-05-23 Martin Pohl

The origin of the extragalactic gamma-ray background (EGRB) is still an open question, even after nearly forty years of its discovery. The emission could originate from either truly diffuse processes or from unresolved point sources.…

高能天体物理现象 · 物理学 2009-11-09 D. Bhattacharya , P. Sreekumar , R. Mukherjee

We investigate whether gamma-ray pulsars viewed at a large angle to the neutron star magnetic pole could contribute to the new population of galactic unidentified EGRET sources associated with the Gould Belt. The faint, soft nature of these…

天体物理学 · 物理学 2009-10-31 Alice K. Harding , Bing Zhang

The nature of the unidentified gamma-ray point sources in the galactic plane is a long standing puzzle of gamma-ray astronomy. Kaaret and Cottam (1996) showed that 16 of the 25 unidentified gamma-ray point sources near the galactic plane…

天体物理学 · 物理学 2007-05-23 Philip Kaaret

Microquasars are X-ray binary systems with non-thermal radio emission originated in jet-like features. They are attractive sites for gamma-ray production, since relativistic particles in the jet should traverse locally strong both photon…

天体物理学 · 物理学 2007-05-23 Gustavo E. Romero

We suggest that ultraluminous X-ray sources (ULXs) and some of the variable low latitude EGRET gamma-ray sources may be two different manifestations of the same underlying phenomena: high-mass microquasars with relativistic jets forming a…

天体物理学 · 物理学 2007-05-23 Yousaf M. Butt , Gustavo E. Romero , Diego F. Torres

Galactic microquasars are certainly one of the most recent additions to the field of high energy astrophysics and have attracted increasing interest over the last decade. However, the high energy part of the spectrum of microquasars is the…

天体物理学 · 物理学 2007-05-23 Josep M. Paredes

The all-sky survey in high-energy gamma rays (E > 30 MeV) carried out by the Energetic Gamma Ray Experiment Telescope (EGRET) aboard the Compton Gamma-Ray Observatory provides a unique opportunity to examine in detail the diffuse gamma-ray…

天体物理学 · 物理学 2011-04-15 Yu. A. Golubkov , M. Yu. Khlopov

In a recent paper, Romero et al. (1999) have presented the results of a positional correlation analysis of the low-latitude unidentified gamma-ray sources in the Third EGRET catalog with complete lists of galactic objects like supernova…

天体物理学 · 物理学 2007-05-23 Gustavo E. Romero , Diego F. Torres , P. Benaglia , J. A. Combi , B. Punsly

The recent detection of a gamma-ray flux from the direction of the Galactic center by EGRET on the Compton GRO raises the question of whether this is a point source (possibly coincident with the massive black hole candidate Sgr A*) or a…

天体物理学 · 物理学 2009-10-30 S. Markoff , F. Melia , I. Sarcevic

We have begun to examine the EGRET database for short term variations in the fluxes of blazars and unidentified sources at high Galactic latitude. We find that several AGN show previously unreported variability. Such variations are…

天体物理学 · 物理学 2009-10-30 S. D. Bloom , D. J. Thompson , R. C. Hartman , C. von Montigny

The large majority of EGRET point sources remain to this day without an identified low-energy counterpart. Whatever the nature of the EGRET unidentified sources, faint unresolved objects of the same class must have a contribution to the…

天体物理学 · 物理学 2008-11-26 V. Pavlidou , J. M. Siegal-Gaskins , C. Brown , B. D. Fields , A. V. Olinto
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