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GRS 1747-312 is a bright transient X-ray source in the globular cluster Terzan 6 with quasi-periodic outbursts approximately every 4.5 months. We carried out 2-60 keV target-of-opportunity observations during eight outbursts with the…

GRS 1747$-$312 is a neutron star Low-Mass X-ray Binary in the globular cluster Terzan 6, located at a distance of 9.5 kpc from the Earth. During its outbursts, periodic eclipses were known to occur. Observations for the outbursts were…

We studied the transient neutron-star low-mass X-ray binary GRS 1747-312, located in the globular cluster Terzan 6, in its quiescent state after its outburst in August 2004, using an archival XMM-Newton observation. A source was detected in…

高能天体物理现象 · 物理学 2018-04-25 Smriti Vats , Rudy Wijnands , Aastha S. Parikh , Laura Ootes , Nathalie Degenaar , Dany Page

GRS 1747-312 is a bright Low-Mass X-ray Binary in the globular cluster Terzan 6, located at a distance of 9.5 kpc from the Earth. It exhibits regular outbursts approximately every 4.5 months, during which periodic eclipses are known to…

Four or five new outbursts were detected of the bright X-ray transient GRS 1747-312 in the globular cluster Terzan 6 between 1996 and 1999, through monitoring campaigns with the Wide Field Cameras (WFCs) on BeppoSAX and the Proportional…

We report a Chandra ACIS-I observation of the dense globular cluster Terzan 5. The previously known transient low-mass x-ray binary (LMXB) EXO 1745-248 in the cluster entered a rare high state during our August 2000 observation,…

天体物理学 · 物理学 2009-11-07 C. O. Heinke , P. D. Edmonds , J. E. Grindlay , D. A. Lloyd , H. N. Cohn , P. M. Lugger

We present a 19 ks Chandra ACIS-S observation of the globular cluster Terzan 1. Fourteen sources are detected within 1.4 arcmin of the cluster center with 2 of these sources predicted to be not associated with the cluster (background AGN or…

We present a short (~3.6 ks) Chandra/HRC-I observation of the globular cluster Terzan 1. This cluster is known to contain the bright neutron star low-mass X-ray binary X 1732-304 which was active during the 1980's and most of the 1990's.…

天体物理学 · 物理学 2009-11-07 Rudy Wijnands , Craig O. Heinke , Jonathan E. Grindlay

We report on Chandra, RXTE, Swift/BAT and MAXI observations of a ~1 day X-ray flare and subsequent outburst of a transient X-ray source observed in October-November 2011 in the globular cluster Terzan 5. We show that the source is the same…

高能天体物理现象 · 物理学 2015-06-05 D. Altamirano , L. Keek , A. Cumming , G. R. Sivakoff , C. O. Heinke , R. Wijnands , N. Degenaar , J. Homan , D. Pooley

EXO 1745-248 is a transient neutron-star low-mass X-ray binary that resides in the globular cluster Terzan 5. We studied the transient during its quiescent state using 18 Chandra observations of the cluster acquired between 2003 and 2016.…

We report our analysis of a Chandra X-ray observation of the rich globular cluster Terzan 5, in which we detect 50 sources to a limiting 1.0-6 keV X-ray luminosity of 3*10^{31} ergs/s within the half-mass radius of the cluster. Thirty-three…

天体物理学 · 物理学 2008-11-26 C. O. Heinke , R. Wijnands , H. N. Cohn , P. M. Lugger , J. E. Grindlay , D. Pooley , W. H. G. Lewin

During a BeppoSAX observation of the X-ray burst source X1732-304 located in the globular cluster Terzan 1 in 1999 April, the source was detected in an anomalously low-state with an X-ray luminosity of 1.4 x 10^33 erg/s$, about 300 times…

天体物理学 · 物理学 2007-05-23 M. Guainazzi , A. N. Parmar , T. Oosterbroek

We report and study the outburst of a new transient X-ray binary (XRB) in Terzan 5, the third detected in this globular cluster, Swift J174805.3-244637 or Terzan 5 X-3. We find clear spectral hardening in Swift/XRT data during the outburst…

We present the results of a search for variability in and near the core of the metal-rich, obscured globular cluster Terzan 5, using NICMOS on HST. This extreme cluster has approximately solar metallicity and a central density that places…

天体物理学 · 物理学 2009-10-31 P. D. Edmonds , J. E. Grindlay , H. N. Cohn , P. M. Lugger

Terzan 5, a globular cluster (GC) prominent in mass and population of compact objects, is searched for diffuse X-ray emission, as proposed by several models. We analyzed the data of an archival Chandra observation of Terzan 5 to search for…

高能天体物理现象 · 物理学 2015-05-18 P. Eger , W. Domainko , A. -C. Clapson

During about 3 years wide field monitoring of the Galactic Center region by the WFC telescopes on board the BeppoSAX satellite, a total of 14 type-I X-ray bursts were detected from the burster 1E 1724-3045 located in the globular cluster…

天体物理学 · 物理学 2009-10-31 M. Cocchi , A. Bazzano , L. Natalucci , P. Ubertini , J. Heise , E. Kuulkers , J. J. M. in 't Zand

We analyze photometry, spectra, and variability of over 100 faint X-ray sources in the globular cluster Terzan 5, using 737 ks of Chandra data. X-ray colors and spectral fitting allow clear separation of foreground sources (with less…

高能天体物理现象 · 物理学 2025-08-05 Gourav Kumawat , Craig O. Heinke , Jiaqi Zhao , Arash Bahramian , Haldan N. Cohn , Phyllis M. Lugger

We present results of the RXTE observations of an extremely intense X-ray burst detected from the source 4U1724-307 in the globular cluster Terzan 2. The burst profile was complex consisting of two precursors and a long primary peak. During…

天体物理学 · 物理学 2007-05-23 S. V. Molkov , S. A. Grebenev , A. A. Lutovinov

Chandra data of the X-ray source [PMH2004] 47 were obtained in the ACIS Survey of M 33 (ChASeM33) in 2006. During one of the observations, the source varied from a high state to a low state and back, in two other observations it varied from…

The X-ray source RX J004717.4-251811 in the nearby starburst galaxy NGC 253 was found to undergo changes from a low to a high state twice, during an XMM-Newton EPIC observation in December 2000 and also during a Chandra observation one year…

天体物理学 · 物理学 2009-11-07 W. Pietsch , F. Haberl , A. Vogler
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