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相关论文: Temporal properties of the short gamma-ray bursts

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A temporal analysis was performed on a sample of 100 bright short GRBs with T90 < 2s from the BATSE Current Catalog along with a similar analysis on 319 long bright GRBs with T90 > 2s from the same catalog. The short GRBs were denoised…

天体物理学 · 物理学 2009-11-07 S. McBreen , F. Quilligan , B. McBreen , L. Hanlon , D. Watson

A comprehensive temporal analysis has been performed on the 319 brightest GRBs with T90>2s from the BATSE current catalog. The rise times, fall times, full-widths at half maximum (FWHM), pulse amplitudes and pulse areas were measured and…

天体物理学 · 物理学 2009-11-07 F. Quilligan , B. McBreen , L. Hanlon , S. McBreen , K. J. Hurley , D. Watson

We analyze the temporal structure of long ((T_{90}>2sec)) and short ((T_{90}<2sec)) BATSE bursts. We find that: (i) In many short bursts (\delta t_{min}/T\ll 1) (where (\delta t_{min}) is the shortest pulse). This indicates that short…

天体物理学 · 物理学 2009-11-06 E. Nakar , T. Piran

The light curves of Gamma-Ray Bursts (GRBs) are believed to result from internal shocks reflecting the activity of the GRB central engine. Their temporal deconvolution can reveal potential differences in the properties of the central…

In order to better understand the physical origin of short duration gamma-ray bursts (GRBs), we perform time-resolved spectral analysis on a sample of 70 pulses in 68 short GRBs with burst duration $T_{90}\lesssim2$ s detected by the…

高能天体物理现象 · 物理学 2020-07-22 Hüsne Dereli-Bégué , Asaf Pe'er , Felix Ryde

Using a theoretical model describing pulse shapes, we have clarified the relations between the observed pulses and their corresponding timescales, such as the angular spreading time, the dynamic time as well as the cooling time. We find…

天体物理学 · 物理学 2008-11-26 Zhibin Zhang , G. Z. Xie , J. G. Deng , B. T. Wei

A sizeable fraction of gamma-ray burst (GRB) time profiles consist of a temporal sequence of pulses. The nature of this stochastic process carries information on how GRB inner engines work. The so-called interpulse time defines the interval…

高能天体物理现象 · 物理学 2014-12-02 A. Baldeschi , C. Guidorzi

We analyze pulse properties of Short gamma-ray bursts (GRBs) from a new catalog containing 434 pulses from 387 BATSE Time-Tagged Event (TTE) GRBs. Short GRB pulses exhibit correlated properties of duration, fluence, hardness, and amplitude,…

高能天体物理现象 · 物理学 2018-03-28 Jon Hakkila , Istvan Horvath , Eric Hofesmann , Stephen Lesage

The temporal properties of a sample of 498 bright gamma-ray bursts (GRBs) with durations between 0.05 s and 674 s were analysed. The large range in duration (T90) is accompanied by a similarly large range in the median values of the pulse…

天体物理学 · 物理学 2009-11-07 S. McBreen , B. McBreen , F. Quilligan , L. Hanlon

We present a simple, semi-analytical model to explain GRB temporal and spectral properties in the context of the internal shock model. Each individual pulse in the temporal profiles is produced by the deceleration of fast moving material by…

天体物理学 · 物理学 2009-11-07 Frederic Daigne , Robert Mochkovitch

We demonstrate that distinguishable gamma-ray burst pulses exhibit similar behaviors as evidenced by correlations among the observable pulse properties of duration, peak luminosity, fluence, spectral hardness, energy-dependent lag, and…

高能天体物理现象 · 物理学 2015-05-27 Jon Hakkila , Robert D. Preece

The prompt emission of Gamma Ray Bursts extends from the early pulses observed in gamma-rays (>15 keV) to very late flares of X-ray photons (0.3-10 keV). The duration of prompt gamma-ray pulses is rather constant while the width of X-ray…

高能天体物理现象 · 物理学 2018-08-01 A. Pescalli , M. Ronchi , G. Ghirlanda , G. Ghisellini

The hard X-ray and gamma-ray phenomenology of gamma-ray bursts (GRBs) can be explained by an external shock model where a single relativistic blast wave interacts with the surrounding medium. Besides reproducing the generic spectral…

天体物理学 · 物理学 2009-10-31 Charles D. Dermer

We have investigated the bimodal distribution of the duration of BATSE gamma-ray bursts (GRBs) by analyzing light curves of 64 ms time resolution. We define the average pulse width of GRBs from the auto-correlation function of GRB profiles.…

天体物理学 · 物理学 2007-05-23 Wenfei Yu , Tipei Li , Mei Wu

We analyze a sample of bright long bursts and find that the pulses duration have a lognormal distribution while the intervals between pulses have an excess of long intervals (relative to lognormal distribution). This excess can be explained…

天体物理学 · 物理学 2009-11-06 Ehud Nakar , Tsvi Piran

Gamma-ray bursts (GRBs) show different behaviours and trends in their spectral evolution. One of the methods used to understand the physical origin of these behaviours is to study correlation between the spectral fit parameters. In this…

高能天体物理现象 · 物理学 2020-06-09 Hüsne Dereli Bégué , Hoi-Fung Yu , Felix Ryde

We have carried out a detailed study of the morphology of gamma-ray bursts (GRBs) with time duration less than 100 ms that includes: (1) a fast-Fourier spectrum analysis, (2) a comparison with the Stern analysis of longer bursts, (3) an…

天体物理学 · 物理学 2009-10-31 David B. Cline , Christina Matthey , Stanislaw Otwinowski

Using the data acquired in the Time To Spill (TTS) mode for long gamma-ray bursts (GRBs) collected by the Burst and Transient Source Experiment on board the Compton Gamma Ray Observatory (BATSE/CGRO), we have carefully measured spectral…

天体物理学 · 物理学 2009-11-10 L. Chen , Y. Q. Lou , M. Wu , J. L. Qu , S. M. Jia , X. J. Yang

Many cosmological models of GRBs envision the energy source to be a cataclysmic stellar event leading to a relativistically expanding fireball. Particles are thought to be accelerated at shocks and produce nonthermal radiation. The highly…

天体物理学 · 物理学 2009-10-31 E. Ramirez-Ruiz , E. E. Fenimore

Currently, the best available probe of the early phase of gamma-ray burst (GRB) jet attributes is the prompt gamma-ray emission, in which several intrinsic and extrinsic variables determine GRB pulse evolution. Bright, usually complex…

天体物理学 · 物理学 2009-11-10 J. P. Norris , J. T. Bonnell , D. Kazanas , J. D. Scargle , J. Hakkila , T. W. Giblin
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