Add to ORKGAbstract. The launch of the Beppo-Sax satellite gave a unique opportunity to investigate gamma ray bursts (GRB) in dierent spectral regions. The large diversity of the afterglow behavior creates additional problems for the cosmological model with a reball. Formation of the afterglow giving the observed diversity of properties is sug-gested in the Galactic neutron star model of GRBs. It is based on the transient accretion disc formation around the neutron star with a low-mass brown companion irradiated by the neutron star. Key words: gamma-ray: bursts 1
We investigated the spectral evolution in the 2-700 keV energy band of gamma-ray bursts (GRBs) detec...
Abstract. We present GRANAT/SIGMA observations of the soft gamma-ray afterglow immediately after the...
8 pages, 5 figures, 4 tablesNew information on short/hard gamma-ray bursts (GRBs) is being gathered ...
The launch of the Beppo-Sax satellite gave a unique opportunity to investigate gamma ray bursts (GRB...
The launch of the Beppo-Sax satellite gave a unique opportunity to investigate gamma ray bursts (GRB...
We provide a comprehensive review of major developments in our understanding of gamma-ray bursts, wi...
I present results from several years of concerted observations of the afterglows and host galaxies o...
GRBs were discovered with the Vela satellites, whose main purpose was to verify compliance with the ...
Context: New information on short/hard gamma-ray bursts (GRBs) is being gathered thanks to the disco...
The merger of a binary of neutron stars provides natural explanations for many of the features of sh...
The discovery of X-ray, optical and radio afterglows of GRBs provides an important tool for understa...
. We consider a jet-disk symbiosis model to explain Gamma Ray Bursts and their afterglows. It is pro...
The galactic model of gamma ray bursts (GRBs) is based upon the observed production of soft gamma ra...
The neutron component is likely an inevitable ingredient of a gamma-ray burst (GRB) baryonic firebal...
Gamma Ray Bursts (GRBs) are short and intense flashes of γ–rays with typical energies between keV an...
We investigated the spectral evolution in the 2-700 keV energy band of gamma-ray bursts (GRBs) detec...
Abstract. We present GRANAT/SIGMA observations of the soft gamma-ray afterglow immediately after the...
8 pages, 5 figures, 4 tablesNew information on short/hard gamma-ray bursts (GRBs) is being gathered ...
The launch of the Beppo-Sax satellite gave a unique opportunity to investigate gamma ray bursts (GRB...
The launch of the Beppo-Sax satellite gave a unique opportunity to investigate gamma ray bursts (GRB...
We provide a comprehensive review of major developments in our understanding of gamma-ray bursts, wi...
I present results from several years of concerted observations of the afterglows and host galaxies o...
GRBs were discovered with the Vela satellites, whose main purpose was to verify compliance with the ...
Context: New information on short/hard gamma-ray bursts (GRBs) is being gathered thanks to the disco...
The merger of a binary of neutron stars provides natural explanations for many of the features of sh...
The discovery of X-ray, optical and radio afterglows of GRBs provides an important tool for understa...
. We consider a jet-disk symbiosis model to explain Gamma Ray Bursts and their afterglows. It is pro...
The galactic model of gamma ray bursts (GRBs) is based upon the observed production of soft gamma ra...
The neutron component is likely an inevitable ingredient of a gamma-ray burst (GRB) baryonic firebal...
Gamma Ray Bursts (GRBs) are short and intense flashes of γ–rays with typical energies between keV an...
We investigated the spectral evolution in the 2-700 keV energy band of gamma-ray bursts (GRBs) detec...
Abstract. We present GRANAT/SIGMA observations of the soft gamma-ray afterglow immediately after the...
8 pages, 5 figures, 4 tablesNew information on short/hard gamma-ray bursts (GRBs) is being gathered ...