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Related papers: A Burst of Speculation

200 papers

We suggest that the collapsing core of a massive rotating star may fragment to produce two or more compact objects. Their coalescence under gravitational radiation gives the resulting black hole or neutron star a significant kick velocity,…

Astrophysics · Physics 2009-11-07 Melvyn B. Davies , Andrew King , Stephan Rosswog , Graham Wynn

From Galactic binary sources, to extragalactic magnetized neutron stars, to long-duration GRBs without associated supernovae, the types of sources we now believe capable of producing bursts of gamma-rays continues to grow apace. With this…

Astrophysics · Physics 2009-06-23 Joshua S. Bloom , Nathaniel R. Butler , Daniel A. Perley

It is conjectured that energy sources of the gamma ray bursts are similar to energy sources which trigger solar and stellar transient activity phenomena like flares, plasma accelerated flows in the flux tubes and, dissipation of energy and…

Solar and Stellar Astrophysics · Physics 2009-09-14 K. M. Hiremath

The clusters of gamma-ray bursts are considered which are assumed to be images of the repeated gamma-ray burst (GRB) sources. It is shown, that localization of the cosmic gamma-ray burst sources (GBS) is determined by the clusters of GRBs.…

Astrophysics · Physics 2007-05-23 A. V. Kuznetsov

We consider a model in which the soft gamma-ray repeaters (SGRs) result from young, magnetized strange stars with superconducting cores. As such a strange star spins down, the quantized vortex lines move outward and drag the magnetic field…

Astrophysics · Physics 2007-05-23 K. S. Cheng , Z. G. Dai

Within the framework of star formation in starburst galaxies undergoing interactions, connections among the red quasars, the BL Lacs, and the Blazars with the gamma-ray bursts are discussed in the light of the "hypernovae" scenario. It is…

Astrophysics · Physics 2007-05-23 Anup Rej

The afterglow emission that follows gamma-ray bursts (GRBs) contains valuable information about the circumburst medium and, therefore, about the GRB progenitor. Theoretical studies of GRB blast waves, however, are often limited to simple…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Petar Mimica , Dimitrios Giannios

The Hubble Space Telescope has recently discovered thousands of gigantic comet-like objects in a ring around the central star in the nearest planetary nebula. We suggest that such circumstellar rings exist around most stars. Collisions of…

Astrophysics · Physics 2008-02-03 Arnon Dar

The detection of two sources of gamma rays towards the microquasar SS 433 has been recently reported. The first source can be associated with SS 433's eastern jet lobe, whereas the second source is variable and displays significant…

High Energy Astrophysical Phenomena · Physics 2020-09-04 Pol Bordas

As it is well-known that the hydrodinamic collapse of the massive star iron core should lead to the production of a hot neutron star. The assumption is made that the thermonuclear burning of the envelope matter, accreting onto the hot…

Astrophysics · Physics 2009-10-31 S. S. Gershtein

One of the most luminous explosions detected, gamma-ray bursts, especially the so-called long-duration bursts, most probably consist of an intrinsic core-collapse to a black hole inside a super massive star. We point out that this collapse…

High Energy Astrophysical Phenomena · Physics 2018-01-23 Antonios Nathanail , Mariafelicia De Laurentis

Several large structures, including the Sloan Great Wall, the Huge Large Quasar Group, and a large gamma-ray burst cluster referred to as the Hercules-Corona Borealis Great Wall, appear to exceed the maximum structural size predicted by…

High Energy Astrophysical Phenomena · Physics 2015-11-18 Istvan Horvath , Zsolt Bagoly , Jon Hakkila , L. Viktor Toth

We explore several models which might be proposed to explain recent possible detections of high-energy (TeV) gamma rays in association with low-energy gamma-ray bursts (GRBs). Likely values (and/or upper limits) for the source energies in…

Astrophysics · Physics 2009-11-07 P. C. Fragile , G. J. Mathews , J. Poirier , T. Totani

It appears that the majority of rapidly-, well-localized gamma-ray bursts with undetected, or dark, optical afterglows, or `dark bursts' for short, occur in clouds of size R > 10L_{49}^{1/2} pc and mass M > 3x10^5L_{49} M_{sun}, where L is…

Astrophysics · Physics 2009-11-07 Daniel E. Reichart , Paul A. Price

The EGRET results for gamma-ray intensities in and near the Galactic Plane have been analysed in some detail. Attention has been concentrated on energies above 1 GeV and the individual intensities in a $4^\circ$ longitude bin have been…

Astrophysics · Physics 2009-11-11 A. D. Erlykin , A. W. Wolfendale

We discuss the possibility that galactic gravitational wave sources might give burst signals at a rate of several events per year, detectable by state-of-the-art detectors. We are stimulated by the results of the data collected by the…

General Relativity and Quantum Cosmology · Physics 2011-08-17 Eugenio Coccia , Florian Dubath , Michele Maggiore

We investigate the number of gamma-ray bursts in two particular strips of the sky using the data in 3B catalog of Burst and Transient Source Experiment (BATSE). One stripe is related to the plane in which the intergalactic globular clusters…

Astrophysics · Physics 2008-02-03 Y. Chen , M. Wu , L. M. Song

In this letter we propose a physical explanation for recently reported correlations between pairs of close and antipodal gamma-ray bursts from publicly available BATSE catalogue. Our model is based on the cosmological scenario in which…

Astrophysics · Physics 2007-05-23 Marek Biesiada

The discovery of strong gamma-ray and hard X-ray emission and the results from various multifrequency campaigns have disclosed new aspects of the blazar phenomenology, leading to a much more robust understanding of the mechanisms underlying…

Astrophysics · Physics 2017-07-12 Gabriele Ghisellini

In a previous work, we have shown that the formation of the Fermi bubbles can be due to the interaction between winds launched from the hot accretion flow in Sgr A* and the interstellar medium (ISM). In that work, we focus only on the…

High Energy Astrophysical Phenomena · Physics 2015-09-23 Guobin Mou , Feng Yuan , Zhaoming Gan , Mouyuan Sun