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相关论文: The Be/X-ray transient KS 1947+300

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Swift J004929.5-733107 is an X-ray source in the Small Magellanic Cloud (SMC) that has been reported several times, but the optical counterpart has been unclear due to source confusion in a crowded region of the SMC. Previous works proposed…

高能天体物理现象 · 物理学 2021-04-21 M. J. Coe , J. A. Kennea , P. A. Evans , L. J. Townsend , A. Udalski , I. M. Monageng , D. A. H. Buckley

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…

天体物理学 · 物理学 2009-11-06 M. J. Coe , I. Negueruela , D. A. H. Buckley , N. J. Haigh , S. G. T. Laycock

I present an optical characterization of the Galactic X-ray transient source MAXI J1957$+$032. This system flares by a factor of $\gtrsim10^{4}$ every few-hundred days, with each flare lasting $\sim5$ days. I identify its quiescent…

高能天体物理现象 · 物理学 2017-12-27 Vikram Ravi

We report the detection of a transient X-ray source toward the Small Magellanic Cloud (SMC) using the X-ray Imaging Spectrometer (XIS) onboard the Suzaku telescope. The source was detected at the edge of the XIS image during a routine…

天体物理学 · 物理学 2017-01-18 D. Takei , M. Tsujimoto , S. Kitamoto , M. Morii , K. Ebisawa , Y. Maeda , E. D. Miller

Soft X-ray transients are systems that are detected when they go into an outburst, wherein their X-ray luminosity increases several orders of magnitude. These outbursts are markers of the poorly understood change in the spectral state of…

高能天体物理现象 · 物理学 2022-02-21 Neal Titus Thomas , Shivappa B. Gudennavar , Ranjeev Misra , Bubbly S. G

We present near infrared (J, H, and K) photometry and moderate resolution (lambda/Deltalambda = 3000) K-band spectroscopy of the embedded stellar cluster in the giant H II region W31. Four of the brightest five cluster members are early…

天体物理学 · 物理学 2009-11-06 R. D. Blum , A. Damineli , P. S. Conti

We study the X-ray transient Swift J1745-26, using observations obtained from its outburst in September 2012, up to its decay towards quiescence in March 2013. We obtained optical and infrared observations, through override programme at…

高能天体物理现象 · 物理学 2020-05-06 Sylvain Chaty , Francis Fortin , Alicia Lopez-Oramas

We report the detection, with HST, of an optical counterpart to the transient supersoft X-ray source 1E 1339.8+2837, in the globular cluster M3. The counterpart is found near the faint end of the subgiant branch in the V vs V-I color…

天体物理学 · 物理学 2009-11-10 Peter D. Edmonds , Peter Kahabka , Craig O. Heinke

The Be star 102719279 is an interesting target observed with CoRoT during two runs, giving us the possibility to study the stability of the detected frequencies and to search for any correlation with outburts, as it was recently found in…

太阳与恒星天体物理 · 物理学 2010-10-12 J. Gutiérrez-Soto , T. Semaan , R. Garrido , F. Baudin , A. -M. Hubert , C. Neiner

We report results from Hubble Space Telescope WFPC2 imaging of the field of the luminous, bursting X-ray source in the globular cluster NGC 6441. Although the X-ray position is known to a precision of a few arcseconds, this source is only…

天体物理学 · 物理学 2009-10-30 Eric W. Deutsch , Scott F. Anderson , Bruce Margon , Ronald A. Downes

Using BATSE and RXTE observations from 1991 April to 2001 August we have detected 71 outbursts from 82 periastron passages of EXO 2030+375, a 42-second transient X-ray pulsar with a Be star companion, including several outbursts from 1993…

天体物理学 · 物理学 2009-11-07 Colleen A. Wilson , Mark H. Finger , M. J. Coe , Silas Laycock , J. Fabregat

We clarify the nature of the small-diameter supernova remnant (SNR) Kes 73 and its central compact source, 1E 1841-045, using X-ray data acquired with the ASCA Observatory. We introduce a spatio-spectral decomposition technique necessary to…

天体物理学 · 物理学 2009-10-30 E. V. Gotthelf , G. Vasisht

We present progenitor-star detections, light curves, and optical spectra of SN2009ip and the 2009 optical transient in UGC2773 (U2773-OT), which were not genuine SNe. Precursor variability in the decade before outburst indicates that both…

An outburst of the X-ray transient source XTE J1806--246 (2S1803--245) has been observed by Rossi X-ray Timing Explorer in April-July 1998. Strong quasi-periodical oscillations (QPO) with a central peak frequency around 9 Hz was detected in…

天体物理学 · 物理学 2007-05-23 M. Revnivtsev , K. Borozdin , A. Emelyanov

We analyze spin-up/spin-down of the neutron star in Be X-ray binary system GX\,304-1 observed by \textit{Swift}/XRT and \textit{Fermi}/GBM instruments in the period of the source activity from April 2010 to January 2013 and discuss possible…

高能天体物理现象 · 物理学 2014-10-31 K. A. Postnov , A. I. Mironov , A. A. Lutovinov , N. I. Shakura , A. Yu. Kochetkova , S. S. Tsygankov

We present K band photometry of the region including the radio error box of the soft X-ray transient 4U 1630-47 during its 1998 outburst. We detect a variable source at K=16.1 mag located inside the radio error circle which we identify as…

天体物理学 · 物理学 2011-03-28 T. Augusteijn , E. Kuulkers , M. H. van Kerkwijk

A fast moving infrared excess source (G2) which is widely interpreted as a core-less gas and dust cloud approaches Sagittarius A* (SgrA*) on a presumably elliptical orbit. VLT K_s-band and Keck K'-band data result in clear continuum…

SAX J1711.6-3808 is an X-ray transient in the Galactic bulge that was active from January through May of 2001 and whose maximum 1-200 keV luminosity was measured to be 5X10-9 erg/s/cm2 which is less than ~25% of the Eddington limit, if…

We present radio observations of the black hole X-ray transient XTE J1720-318, which was discovered in 2003 January as it entered an outburst. We analyse the radio data in the context of the X-ray outburst and the broad-band spectrum. An…

天体物理学 · 物理学 2009-11-10 C. Brocksopp , S. Corbel , R. P. Fender , M. Rupen , R. Sault , S. J. Tingay , D. Hannikainen , K. O'Brien

This paper reports the discovery of a bright X-ray transient source, Suzaku J1305-4913, in the south-west arm of the nearby Seyfert II galaxy NGC 4945. It was detected at a 0.5 -- 10 keV flux of $2.2 \times 10^{-12}$ erg cm$^{-2}$ s$^{-1}$…

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