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Twenty-two extragalactic fast X-ray transients (FXTs) have now been discovered from two decades of Chandra data (analyzing ~259 Ms of data), with 17 associated with distant galaxies (>100 Mpc). Different mechanisms and progenitors have been…

Fast X-ray transients (FXTs) are bright X-ray flashes with durations of minutes to hours, peak isotropic luminosities of L_X,peak ~ 10^42-10^47 erg/s, and total isotropic energies of E ~ 10^47-10^50 erg. They have been detected in the soft…

高能天体物理现象 · 物理学 2025-08-28 Sumedha Biswas , Peter G. Jonker , M. Coleman Miller , Andrew Levan , Jonathan Quirola-Vásquez

The observed light curves and other properties of the two extragalactic fast x-ray transients, CDF-S XT1 and CDF-S XT2, which were discovered recently in archival data of the Chandra Deep Field-South (CDF-S) observations, indicate that they…

高能天体物理现象 · 物理学 2020-03-11 Shlomo Dado , Arnon Dar

Neutron star-neutron star mergers are known to be associated with short gamma-ray bursts. If the neutron star equation of state is sufficiently stiff, at least some of such mergers will leave behind a supramassive or even a stable neutron…

高能天体物理现象 · 物理学 2019-04-12 Y. Q. Xue , X. C. Zheng , Y. Li , W. N. Brandt , B. Zhang , B. Luo , B. B. Zhang , F. E. Bauer , H. Sun , B. D. Lehmer , X. F. Wu , G. Yang , X. Kong , J. Y. Li , M. Y. Sun , J. -X. Wang , F. Vito

Extragalactic Fast X-ray Transients (FXRTs) are short flashes of X-ray photons spanning a few seconds to hours, with an uncertain origin. Our ignorance about their physical mechanisms and progenitor systems is due in part to the lack of…

高能天体物理现象 · 物理学 2022-08-03 J. Quirola-Vasquez , F. E. Bauer , P. G. Jonker , W. N. Brandt , G. Yang , A. J. Levan , Y. Q. Xue , D. Eappachen , X. C. Zheng , B. Luo

Extragalactic fast X-ray transients (FXTs) are short flashes of X-ray photons of unknown origin that last a few minutes to hours. We extend the search for extragalactic FXTs from Quirola et al. 2022 (Paper I; based on sources in the Chandra…

Two bright X-ray transients were reported from the Chandra Deep Field South archival data, namely CDF-S XT1 and XT2. Whereas the nature of the former is not identified, the latter was suggested as an excellent candidate for a rapidly…

高能天体物理现象 · 物理学 2019-12-03 Hui Sun , Ye Li , Binbin Zhang , Bing Zhang , Franz E. Bauer , Yongquan Xue , Weimin Yuan

Recent works have discovered two fast ($\approx 10$ ks) extragalactic X-ray transients in the Chandra Deep Field-South (CDF-S XT1 and XT2). These findings suggest that a large population of similar extragalactic transients might exist in…

高能天体物理现象 · 物理学 2019-06-19 Guang Yang , W. N. Brandt , S. F. Zhu , F. E. Bauer , B. Luo , Y. Q. Xue , X. C. Zheng

Fast X-ray Transients (FXTs) are X-ray flares with a duration ranging from a few hundred seconds to a few hours. Possible origins include the tidal disruption of a white dwarf by an intermediate-mass black hole, a supernova shock breakout,…

Fast X-ray transients (FXTs) are flashes of X-rays that last for a few hundreds of seconds to a few hours. An enigmatic population of these transients that did not have a clear origin has been known for several decades, mostly found…

高能天体物理现象 · 物理学 2026-01-22 Murray Brightman , Joahan Castañeda Jaimes , Daniel Stern , Brian Grefenstette

Extragalactic fast X-ray transients (FXTs) are a class of soft (0.3-10 keV) X-ray transients lasting a few hundred seconds to several hours. Several progenitor mechanisms have been suggested to produce FXTs, including supernova shock…

In this paper we summarize some aspects of the wind accretion theory in high mass X-ray binaries hosting a magnetic neutron star and a supergiant companion. In particular, we concentrate on the different types of interaction between the…

天体物理学 · 物理学 2008-11-07 E. Bozzo , M. Falanga , L. Stella

Over the past few years, $\sim$30 extragalactic fast X-ray transients (FXRTs) have been discovered, mainly in Chandra and XMM-Newton data. Their nature remains unclear, with proposed origins including a double neutron star merger, a tidal…

XRT 201423 is an X-ray transient with a nearly flat plateau lasting 4.1 ks followed by a steep decay. This feature indicates that it might come from a magnetar formed through a binary neutron star merger, similar to CDF-S XT2 and as…

高能天体物理现象 · 物理学 2021-07-07 Shunke Ai , Bing Zhang

Fast X-ray transients (FXTs) are X-ray flares lasting minutes to hours. Multi-wavelength counterparts to these FXTs have been proven hard to find. As a result distance measurements are through indirect methods such as host galaxy…

高能天体物理现象 · 物理学 2024-09-25 Anne Inkenhaag , Peter G. Jonker , Andrew J. Levan , Jonathan Quirola-Vásquez , Franz E. Bauer , Deepak Eappachen

Very recently \citet{XueYQ2019} reported an important detection of the X-ray transient, CDF-S XT2, whose light curve is analogous to X-ray plateau features of gamma-ray burst afterglows. They suggested that this transient is powered by a…

高能天体物理现象 · 物理学 2019-07-10 Di Xiao , Bin-Bin Zhang , Zi-Gao Dai

We present a novel representation learning method for downstream tasks like anomaly detection, unsupervised classification, and similarity searches in high-energy data sets. This enabled the discovery of a new extragalactic fast X-ray…

高能天体物理现象 · 物理学 2025-03-05 Steven Dillmann , Juan Rafael Martínez-Galarza , Roberto Soria , Rosanne Di Stefano , Vinay L. Kashyap

The low luminosity, X-ray flaring activity, of the sub-class of high mass X-ray binaries called Supergiant Fast X-ray Transients, has been investigated using XMM-Newton public observations, taking advantage of the products made publicly…

高能天体物理现象 · 物理学 2019-05-15 L. Sidoli , K. A. Postnov , A. Belfiore , M. Marelli , D. Salvetti , R. Salvaterra , A. De Luca , P. Esposito

Supergiant Fast X-ray Transients (SFXTs) are one of the most intriguing (and unexpected) results of the INTEGRAL mission. They are a new class of High Mass X-ray Binaries involving about 20 sources to date, with 8 firmly identified SFXTs…

天体物理仪器与方法 · 物理学 2010-01-20 L. Sidoli , V. Sguera , A. Bazzano , P. Ubertini

Supergiant fast X-ray transients (SFXTs) are high mass X-ray binaries (HMXBs) hosting a neutron star and an OB supergiant companion. We examine the available Swift data, as well as other new or archival/serendipitous data, on three sources:…

高能天体物理现象 · 物理学 2016-10-05 P. Romano , E. Bozzo , P. Esposito , B. Sbarufatti , F. Haberl , G. Ponti , P. D'Avanzo , L. Ducci , A. Segreto , C. Jin , N. Masetti , M. Del Santo , S. Campana , V. Mangano
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