2000A&A...364..552P


Query : 2000A&A...364..552P

2000A&A...364..552P - Astronomy and Astrophysics, volume 364, 552-556 (2000/12-2)

An inquiry into the nature of the gamma-ray source 3EG J1828+0142.

PUNSLY B., ROMERO G.E., TORRES D.F. and COMBI J.A.

Abstract (from CDS):

The unidentified, low-latitude, γ-ray source 3EG J1828+0142 presents high levels of variability and a steep spectral index Γ∼2.7. Here we propose a model for this source where the high-energy emission is produced by a galactic Kerr-Newman black hole. The model takes into account electron-positron annihilation losses in the calculation of the expected spectral energy distribution and can reproduce the observational features, including the absence of a strong radio counterpart. We also report the discovery of a nearby supernova remnant that could be associated with the original supernova explosion that created the black hole. Several faint radio sources were also detected in the radio field within the inner γ-ray confidence contour and their spectral index estimated. Some of these sources could be the expected weak radio counterpart.

Abstract Copyright:

Journal keyword(s): gamma rays: theory - gamma rays: observations - radio continuum: ISM - ISM: supernova remnants - black hole physics

Nomenclature: Fig.1, Table 2: [PRT2000] SN (Nos S1-S4).

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 TXS 1825+016 Rad 18 28 25.8 +01 39 53           ~ 1 0
2 [PRT2000] S2 Rad 18 28.6 +01 45           ~ 1 0
3 [PRT2000] S4 Rad 18 28.7 +01 34           ~ 1 0
4 GRO J1834+01 gam 18 29 +01.7           ~ 20 0
5 [PRT2000] S3 Rad 18 29.4 +01 45           ~ 1 0

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2022.05.23-10:23:47

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