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We have extended our earlier study (Heard & Warwick 2013, Paper I) of the X-ray emission emanating from the central 100 pc x 100 pc region of our Galaxy to an investigation of several features prominent in the soft X-ray (2-4.5 keV) band.…

High Energy Astrophysical Phenomena · Physics 2015-06-16 V. Heard , R. S. Warwick

If typical gamma-ray bursts (GRBs) have X-ray counterparts similar to those detected by Ginga, then sensitive focusing X-ray telescopes will be able to detect GRBs three orders of magnitude fainter than the detection limit of the Burst and…

Astrophysics · Physics 2009-10-28 T. T. Hamilton , E. V. Gotthelf , D. J. Helfand

We perform two-dimensional hydrodynamical simulations of slowly rotating accretion flows in the region of $ 0.01-7\, \mathrm{pc} $ around a supermassive black holes with $ M_\mathrm{BH} = 10^{8} M_{\odot} $. The accretion flow is irradiated…

High Energy Astrophysical Phenomena · Physics 2019-10-23 Amin Mosallanezhad , Feng Yuan , Jeremiah P. Ostriker , Fatemeh Zahra Zeraatgari , De-Fu Bu

Blazars radiate from relativistic plasma jets with bulk Lorentz factors {\Gamma} ~ 10, closely aligned along our line of sight. In a number of blazars of the Flat Spectrum Radio Quasar type such as 3C 454.3 and 3C 279 gamma-ray flares have…

High Energy Astrophysical Phenomena · Physics 2015-10-22 Marco Tavani , Valerio Vittorini , Alfonso Cavaliere

Relativistic outflows with neutrons inevitably lead to inelastic collisions, and resulting subphotospheric gamma rays may explain prompt emission of gamma-ray bursts. In this model, hadronuclear, quasithermal neutrinos in the 10-100 GeV…

High Energy Astrophysical Phenomena · Physics 2013-10-01 Kohta Murase , Kazumi Kashiyama , Peter Meszaros

I calculate spectral evolution series for pulses of GRBs, in the BATSE spectral range, for continuous particle injection and cooling by synchrotron, inverse Compton, and adiabatic expansion. The hydrodynamic properties of the relativistic…

Astrophysics · Physics 2009-10-31 H. Papathanassiou

When a star undergoes core collapse, a vast amount of energy is released in a ~10 s long burst of neutrinos of all species. Inverse beta decay in the star's hydrogen envelope causes an electromagnetic cascade which ultimately results in a…

High Energy Astrophysical Phenomena · Physics 2024-08-06 Cecilia Lunardini , Joshua Loeffler , Mainak Mukhopadhyay , Matthew J. Hurley , Ebraheem Farag , F. X. Timmes

Many classes of gamma-ray sources, such as gamma-ray bursts, blazars, Seyfert galaxies, and galactic black hole sources are surrounded by large amounts of gas and dust. X-rays and gamma-rays that traverse this material will be attenuated by…

Astrophysics · Physics 2007-05-23 C. D. Dermer , M. Boettcher , E. P. Liang

An electron-positron atmosphere is inevitably created around a black hole accretion disc, the spectrum of which extends to MeV energies. Pairs created in photon-photon collisions outside the disc are blown away by soft radiation (which…

Astrophysics · Physics 2009-10-31 Andrei M. Beloborodov

We investigate the angular distribution of the $\gamma$-ray bursts in the publicly available BATSE catalogue, using the measures of burst brightness $B$ and short time scale ($\simless$ 0.3 s) variability $V$ which we introduced earlier. We…

Astrophysics · Physics 2016-06-08 J. M. Quashnock , D. Q. Lamb

X-ray absorption and emission lines now serve as powerful diagnostics of the outflows from active galaxies. Detailed X-ray line studies of outflows have recently been enabled for a significant number of active galaxies via the grating…

Astrophysics · Physics 2009-11-07 W. N. Brandt , S. Kaspi

We test the models of synchrotron emission presented in Part I of this series (Lloyd & Petrosian, these proceedings) against the distributions and evolution of GRB spectral parameters (particularly the low energy index, $\alpha$). With…

Astrophysics · Physics 2018-11-06 Nicole M. Lloyd-Ronning , Vahe' Petrosian , Robert D. Preece

Relativistic bulk motion with large Lorentz factors has recently been inferred for gamma-ray bursts regardless of whether they are of galactic or cosmological origin. This conclusion results from calculations of internal pair production…

Astrophysics · Physics 2009-10-30 Matthew G. Baring , Alice K. Harding

Bursts from soft gamma repeaters have been shown to be super-Eddington by a factor of 1000 and have been persuasively associated with compact objects. Here, a model of super-Eddington radiation transfer on the surface of a strongly magnetic…

Astrophysics · Physics 2009-10-22 Andrew Ulmer

The blast-wave model for gamma-ray bursts (GRBs) has been called into question by observations of spectra from GRBs that are harder than can be produced through optically thin synchrotron emission. If GRBs originate from the collapse of…

Astrophysics · Physics 2009-10-31 Charles D. Dermer , Markus Boettcher

Recent results of the hectic research activity about gamma-ray bursts will be reviewed, with emphasis about the emission processes at the origin of the observed gamma-rays. The conventional synchrotron shock scenario is found to have…

Astrophysics · Physics 2007-05-23 Gabriele Ghisellini

We investigate starburst-driven galactic outflows in low-mass galaxies ($9.0 < \log(M_*/M_\odot) < 10.0$) at cosmic noon using high-resolution 3D hydrodynamical simulations based on a framework that can reproduce the multiphase outflows in…

Astrophysics of Galaxies · Physics 2026-02-10 Huan Chen , Weishan Zhu , Xue-Fu Li , Tian-Rui Wang , Antonios Katsianis , Long-Long Feng

Galactic outflows play a major role in the evolution of galaxies, but the underlying physical processes are poorly understood. This is mainly because we have little information about the outflow structure, especially on large scales. In…

Astrophysics of Galaxies · Physics 2020-05-19 Bingjie Wang , Timothy M. Heckman , Guangtun Zhu , Colin A. Norman

Central molecular outflows in spiral galaxies are assumed to modulate their host galaxy's star formation rate by removing gas from the inner region of the galaxy. Outflows consisting of different gas phases appear to be a common feature in…

If the emission of gamma-ray bursts were due to the synchrotron process in the standard internal shock scenario, then the typical observed spectrum should have a slope F(nu) \propto nu^{-1/2}, which strongly conflicts with the much harder…

Astrophysics · Physics 2009-10-31 Gabriele Ghisellini , Annalisa Celotti , Davide Lazzati
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