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Related papers: RX J1420.4+5334 - another tidal disruption event?

200 papers

Active galactic nuclei (AGN), powered by long-term accretion onto central supermassive black holes, produce relativistic jets with lifetimes of greater than one million yr that preclude observations at birth. Transient accretion onto a…

We present the discovery of the first X-ray counterpart to a Rotating RAdio Transient (RRAT) source. RRAT J1819--1458 is a relatively highly magnetized (B $\sim 5\times10^{13}$ G) member of a new class of unusual pulsar-like objects…

We present multiwavelength studies of a transient X-ray source, XMMSL1 J131952.3+225958, associated with the galaxy NGC 5092 at $z=0.023$ detected in the XMM-Newton SLew survey (XMMSL). The source brightened in the 0.2--2 keV band by a…

High Energy Astrophysical Phenomena · Physics 2020-03-23 Dongyue Li , R. D. Saxton , Weimin Yuan , Luming Sun , He-Yang Liu , Ning Jiang , Huaqing Cheng , Hongyan Zhou , S. Komossa , Chichuan Jin

Theory suggests that a star making a close passage by a supermassive black hole at the center of a galaxy can under most circumstances be expected to emit a giant flare of radiation as it is disrupted and a portion of the resulting stream…

High Energy Astrophysical Phenomena · Physics 2010-11-17 Peter Maksym , Melville P. Ulmer , Michael Eracleous

XTE J1701-462 is a neutron star low mass X-ray binary (NS LMXB) discovered in 2006 as the first system to demonstrate unambiguously that the `Atoll' and `Z' classes of accreting neutron stars are separated by accretion rate. Radio…

High Energy Astrophysical Phenomena · Physics 2024-08-01 K. V. S. Gasealahwe , I. M. Monageng , R. P. Fender , P. A. Woudt , A. K. Hughes , S. E. Motta , J. van den Eijnden , P. Saikia , E. Tremou

We report on continued monitoring observations of the Galactic center carried out by the X-ray telescope aboard the Swift satellite in 2008 and 2009. This campaign revealed activity of the five known X-ray transients AX J1745.6-2901, CXOGC…

High Energy Astrophysical Phenomena · Physics 2015-05-19 N. Degenaar , R. Wijnands

We report a discovery of strong modulations of the X-ray flux detected from IGR J16320-4751 = AX J1631.9-4752 with a period of P~1300 sec. We reanalyzed the data of an XMM-Newton ToO performed soon after the discovery of the source by…

Astrophysics · Physics 2009-11-10 A. Lutovinov , J. Rodriguez , M. Revnivtsev , P. Shtykovskiy

We investigated the optical, X-ray, and gamma-ray variability of the pulsar SAX J2103.5+4545. Our timing and spectral analyses of the X-ray and gamma-ray emissions from the source using RXTE and INTEGRAL data show that the shape of its…

We present further observational data of the supersoft X-ray source RX J0527.8-6954 exhibiting a continuous decline over the past 5 yrs. With no clear trend of a concordant temperature decrease this might suggest an evolutionary scenario…

Astrophysics · Physics 2007-05-23 J. Greiner , R. Schwarz , G. Hasinger , M. Orio

Two optical candidates - a galaxy and a star, are found within the error circle of the X-ray source position of an ultra-soft X-ray source discovered with ROSAT. Optical spectroscopy of the two candidates reveals that a) the galaxy is a…

Astrophysics · Physics 2007-05-23 Kulinder Pal Singh , Laurence R. Jones

We present a sample of 47 spectroscopically confirmed members of RX J1347-1145, the most luminous X-ray cluster of galaxies discovered to date. With two exceptions, all the galaxies in this sample have red B-R colors and red spectral…

Astrophysics · Physics 2009-11-07 Judith G. Cohen , Jean-Paul Kneib

The recently discovered J0651+2844 is a detached, eclipsing white dwarf binary with an orbital period of 765 s. We investigate the prospects for the detection of gravitational radiation from this system and estimate the effect of the tidal…

Solar and Stellar Astrophysics · Physics 2015-05-30 Matthew Benacquista

We studied the X-ray timing and spectral variability of the X-ray source Sw J1644+57, a candidate for a tidal disruption event. We have separated the long-term trend (an initial decline followed by a plateau) from the short-term dips in the…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Curtis J. Saxton , Roberto Soria , Kinwah Wu , N. Paul M. Kuin

A new pulsating X-ray source, AX J183220-0840, with a 1549.1-s period was discovered at R.A.= 18h32m20s and Dec.=-8d40'30'' (J2000, uncertainty=0.6degree) during an ASCA observation on the Galactic plane. The source was observed two times,…

Astrophysics · Physics 2009-10-31 M. Sugizaki , K. Kinugasa , K. Matsuzaki , Y. Terada , S. Yamauchi , J. Yokogawa

We report the discovery of an off-nuclear ultrasoft hyper-luminous X-ray source candidate 3XMM J141711.1+522541 in the inactive S0 galaxy SDSS J141711.07+522540.8 (z=0.41827, d_L=2.3 Gpc) in the Extended Groth Strip. It is located at a…

We report the discovery of a new isolated neutron star candidate, RX J0420.0-5022, showing evidence (4 sigma) for 22.7 s X-ray pulsations in ROSAT data. NTT observations of the field around the soft X-ray source do not reveal any likely…

Astrophysics · Physics 2007-05-23 F. Haberl , W. Pietsch , C. Motch

An unusual double-lobed extended X-ray source (RX J105343+5735) is detected in the ROSAT ultra-deep HRI image of the Lockman Hole. The angular size of the source is 1.7 X 0.7 arcmin^2 and its X-ray flux is 2 X 10^-14 erg cm^-2 s^-1. R-band…

We report observations which confirm the identities of the optical counterpart to the transient sources RX J0544.1-7100 and RX J0520.5-6932. The counterparts are suggested to be a B-type stars. Optical data from the observations carried out…

Astrophysics · Physics 2009-11-06 M. J. Coe , I. Negueruela , D. A. H. Buckley , N. J. Haigh , S. G. T. Laycock

We report the discovery of the X-ray transient SAX J2103.5+4545 which was active from February to September 1997. The observed peak intensity of 20 mCrab (2 to 25 keV) occurred on April 11. An analysis of data obtained around the time of…

Astrophysics · Physics 2007-05-23 F. Hulleman , J. J. M. in 't Zand , J. Heise

We present the results from the multi-wavelength monitoring observations of the Narrow-Line Seyfert 1 galaxy Mrk 335 with AstroSat. We analysed both the X-ray (SXT & LAXPC) and UV (UVIT) data of the source at two epochs, separated by ~18…

High Energy Astrophysical Phenomena · Physics 2021-06-30 Savithri H. Ezhikode , Gulab C. Dewangan , Ranjeev Misra