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相关论文: X-ray flashes from off-axis nonuniform jets

200 篇论文

We calculate the spectra expected from unsteady relativistic wind models of gamma-ray bursts, suitable for events of arbitrary duration. The spectral energy distribution of the burst is calculated over photon energies spanning from eV to…

天体物理学 · 物理学 2009-10-28 Hara Papathanassiou , Peter Meszaros

Although the gamma-ray emission in blazars dominates the power output, there are crucial informations carried by the X-rays. Indeed, their paucity, together with the short variability timescales observed both at X and gamma-ray energies…

天体物理学 · 物理学 2007-05-23 Gabriele Ghisellini

We present a comparison of the parameters of accretion disc outflows and the jet of the broad-line radio galaxy 3C 111 on sub-pc scales. We make use of published X-ray observations of ultra-fast outflows (UFOs) and new 43GHz VLBA images to…

高能天体物理现象 · 物理学 2015-06-05 F. Tombesi , R. M. Sambruna , A. P. Marscher , S. G. Jorstad , C. S. Reynolds , A. Markowitz

Gamma-ray emission from AGN provides us with unprecedented insights into the physics of extragalactic jets. The emission from these jets fits naturally into the existing theoretical framework of relativistic jets as inferred from parsec…

天体物理学 · 物理学 2009-11-06 G. V. Bicknell , S. J. Wagner , B. A. Groves

We discuss morphological properties of the large-scale jets in powerful radio sources, which are now observed at radio, optical and X-ray frequencies, in order to determine the origin of their X-ray radiation and the nature of the particle…

天体物理学 · 物理学 2009-11-10 L. Stawarz , M. Sikora , M. Ostrowski , M. C. Begelman

X-shaped Radio Galaxies (XRGs) develop when certain extra-galactic jets deviate from their propagation path. An asymmetric ambient medium (Back-flow model) or complex Active Galactic Nuclei activity (Jet-reorientation model) enforcing the…

星系天体物理 · 物理学 2023-08-01 Gourab Giri , Bhargav Vaidya , Christian Fendt

Using new deep VLA and HST observations of the large-scale jet in 3C273 matched to 0.3" resolution, we have detected excess near-ultraviolet emission (300 nm) above a synchrotron cutoff spectrum accounting for the emission from radio…

天体物理学 · 物理学 2009-11-07 S. Jester , H. -J. Roeser , K. Meisenheimer , R. Perley

We show that there is no universal law describing how the spectra and luminosity of synchrotron and inverse Compton radiation from relativistic jets change with increasing observation angle. Instead, the physics of particle acceleration…

天体物理学 · 物理学 2008-11-26 E. V. Derishev , F. A. Aharonian , Vl. V. Kocharovsky

In the past two years, tremendous progresses to understand X-ray Flashes have been made. Now it is widely believed that X-ray Flashes and Gamma-ray Bursts are intrinsically the same, their much different peak energy and flux may be just due…

天体物理学 · 物理学 2009-11-10 Y. Z. Fan , D. M. Wei , C. F. Wang

X-ray binaries are binary star systems in which a compact object (a neutron star or a black hole) and a relatively normal star orbit a common centre of mass. Since the discovery of X-ray binaries with the first X-ray telescopes in the…

天体物理学 · 物理学 2008-02-07 David Russell

The degree and the temporal evolution of linear polarization in the prompt and afterglow emission of gamma-ray bursts is a very robust diagnostic of some key features of gamma-ray bursts jets and their micro and macro physics. In this…

高能天体物理现象 · 物理学 2016-06-01 Davide Lazzati

We discuss production of very high energy (VHE) gamma-rays in large scale extragalactic jets of FR I sources. Based on recent optical and X-ray observations of these objects we evaluate their VHE emission in a framework of one electron…

天体物理学 · 物理学 2007-05-23 L. Stawarz , M. Ostrowski , M. Sikora

Gamma-ray bursts (GRBs) are known to be highly collimated events, and are mostly detectable when they are seen on-axis or very nearly on-axis. However, GRBs can be seen from off-axis angles, and the recent detection of a short GRB…

高能天体物理现象 · 物理学 2021-02-03 Ruben Farinelli , Rupal Basak , Lorenzo Amati , Cristiano Guidorzi , Filippo Frontera

Most of the hadronic jet models for quasars (QSOs) and microquasars (MQs) found in literature represent beams of particles (e.g. protons). These particles interact with the matter in the stellar wind of the companion star in the system or…

高能天体物理现象 · 物理学 2015-05-27 Diego F. Torres , Anita Reimer

Nonthermal radiation observed from astrophysical systems containing relativistic jets and shocks, e.g., gamma-ray bursts (GRBs), active galactic nuclei (AGNs), and Galactic microquasar systems usually have power-law emission spectra. Recent…

We report on new X-ray observations of the large-scale jets recently discovered in X-rays from the black hole candidate 4U 1755-33. Our observations in 2004 show that the jets found in 2001 are still present in X-rays. However, sensitive…

天体物理学 · 物理学 2008-11-26 P. Kaaret , S. Corbel , J. A. Tomsick , J. Lazendic , A. K. Tzioumis , Y. Butt , R. Wijnands

Extragalactic fast X-ray transients (FXTs) are short-duration ($\sim$ ks) X-ray flashes of unknown origin, potentially arising from binary neutron star mergers. We investigate the possible link between FXTs and the afterglows of off-axis…

高能天体物理现象 · 物理学 2024-07-10 H. C. I. Wichern , M. E. Ravasio , P. G. Jonker , J. A. Quirola-Vásquez , A. J. Levan , F. E. Bauer , D. A. Kann

The X-ray emission mechanism of powerful extragalactic jets, which has important implications for their environmental impact, is poorly understood. The X-ray/radio positional offsets in individual features of jets provide important clues.…

高能天体物理现象 · 物理学 2023-03-01 Karthik Reddy , Markos Georganopoulos , Eileen T. Meyer , Mary Keenan , Kassidy E. Kollman

Gamma-ray burst (GRB) jets are narrow, and thus typically point away from us. They are initially ultra-relativistic, causing their prompt $\gamma$-ray and early afterglow emission to be beamed away from us. However, as the jet gradually…

高能天体物理现象 · 物理学 2018-09-19 Jonathan Granot , Fabio De Colle , Enrico Ramirez-Ruiz

We present a general method for testing gamma-ray burst (GRB) jet structure and carry out a comprehensive analysis about the prevalent jet structure models. According to the jet angular energy distribution, we can not only derive the…

天体物理学 · 物理学 2009-11-13 L. Xu , X. F. Wu , Z. G. Dai