English
Related papers

Related papers: The MAVERIC survey: A transitional millisecond pul…

200 papers

We report the timing analysis results of X-ray pulsars from a recent deep Chandra survey of the Small Magellanic Cloud (SMC). We have analyzed a total exposure of 1.4 Ms from 31 observations over a 1.2 deg$^2$ region in the SMC under a…

High Energy Astrophysical Phenomena · Physics 2017-10-04 JaeSub Hong , Vallia Antoniou , Andreas Zezas , Frank Haberl , Manami Sasaki , Jeremy Drake , Paul Plucinsky , Silas Laycock

We have identified an X-ray transient (hereafter M15 X-3) in the globular cluster M15 from an archival Chandra grating observation. M15 X-3 appears at an X-ray luminosity of 6*10^{33} ergs/s with a spectrum consistent with an absorbed power…

Astrophysics · Physics 2010-07-28 Craig O. Heinke , Haldan N. Cohn , Phyllis M. Lugger

We report on the results obtained for the millisecond transient X-ray pulsar XTE J1807-294 in a 40 min orbital period system, based on an XMM-Newton ToO observation carried out during March 2003. The source was found at a luminosity level…

Astrophysics · Physics 2009-11-10 S. Campana , M. Ravasio , G. L. Israel , V. Mangano , T. Belloni

We present the results of a pair of 100 ksec Chandra observations in the Small Magellanic Cloud to survey high mass X-ray binaries (HMXBs), stars and LMXBs/CVs down to Lx = 4.3 x 10^32 erg/s The two SMC Deep Fields are located in the most…

Astrophysics · Physics 2014-08-05 Silas Laycock , Andreas Zezas , Jaesub Hong , Jeremy Drake , Valsamo Antoniou

SAX J1748.9-2021 is a transiently accreting X-ray millisecond pulsar. It is also known as an X-ray burster source discovered by Beppo-SAX. We analysed the persistent emission and type-I X-ray burst properties during its 2015 outburst. The…

High Energy Astrophysical Phenomena · Physics 2018-12-12 Zhaosheng Li , V. De Falco , M. Falanga , E. Bozzo , L. Kuiper , J. Poutanen , A. Cumming , D. K. Galloway , Shu Zhang

Using the Chandra/ACIS-I detector, we have identified an X-ray source (CXOU 132619.7-472910.8) in the globular cluster NGC 5139 with a thermal spectrum identical to that observed from transiently accreting neutron stars in quiescence. The…

We report the discovery of a fairly bright transient during observations with the Wide Field Cameras on board the BeppoSAX satellite in September 1996. It was detected at a peak intensity of 0.1 Crab (2 to 10 keV) and lasted between 6 and…

Astrophysics · Physics 2008-11-26 J. J. M. in 't Zand , J. Heise , J. M. Muller , A. Bazzano , M. Cocchi , L. Natalucci , P. Ubertini

MeerKAT imaging of the globular cluster 47 Tucanae (47 Tuc) reveals 1.28 GHz continuum emission at the locations of 20 known millisecond pulsars (MSPs). We use time series and spectral imaging to investigate the image-domain characteristics…

High Energy Astrophysical Phenomena · Physics 2023-07-19 Ian Heywood

The results of ART-P/Granat observations of the X-ray burster SLX1732-304 in the globular cluster Terzan 1 are presented. The X-ray (3-20 keV) fluxes from the source differed by more than a factor of 4 during the observing sessions on…

Astrophysics · Physics 2009-11-06 M. N. Pavlinsky , S. A. Grebenev , A. A. Lutovinov , R. A. Sunyaev , A. V. Finoguenov

Two sensitive Chandra X-ray observations of the heavily-reddened galactic starburst cluster Westerlund 1 in May and June 2005 detected a previously unknown X-ray pulsar (CXO J164710.20-455217). Its slow 10.6 s pulsations, moderate X-ray…

Astrophysics · Physics 2008-11-26 S. L. Skinner , R. Perna , S. A. Zhekov

Diffuse X-ray emission has been detected from a few Galactic globular clusters (GCs), whereas its nature still remains largely unclear. The GC Terzan 5 was previously found to show a significant diffuse thermal X-ray excess from its field,…

High Energy Astrophysical Phenomena · Physics 2025-01-15 Jiaqi Zhao , Craig O. Heinke , Su Fu

XMM-Newton and Chandra observations of the transient 7.8 s pulsar XTE J1829-098 are used to characterize its pulse shape and spectrum, and to facilitate a search for an optical or infrared counterpart. In outburst, the absorbed, hard X-ray…

Astrophysics · Physics 2009-11-13 J. P. Halpern , E. V. Gotthelf

Millisecond pulsars (MSPs) are thought to born in low-mass X-ray binaries when the neutron star has gained enough angular momentum from the accreting materials of its companion star. It is generally believed that a radio MSP is born when…

High Energy Astrophysical Phenomena · Physics 2014-12-17 P. H. T. Tam , K. L. Li , A. K. H. Kong , J. Takata , G. C. K. Leung , K. S. Cheng , C. Y. Hui

We present a multi-band search for X-ray, optical and $\gamma$-ray emission of the radio binary millisecond pulsar J1836-2354A, hosted in the globular cluster M22. X-ray emission is significantly detected in two Chandra observations,…

High Energy Astrophysical Phenomena · Physics 2019-04-24 R. Amato , A. D'Aì , M. Del Santo , D. de Martino , A. Marino , T. Di Salvo , R. Iaria , T. Mineo

We report on a BeppoSAX observation of the transient X-ray pulsar 4U 0115+63 close to periastron. This led to the discovery of a dramatic luminosity variation from ~2x10^34 erg/s to ~5x10^36 erg/s (factor ~250) in less than 15 hr. The…

We present the results of a search for X-ray variability in the galactic open cluster NGC 2516. This cluster has been observed on 8 occasions using XMM-Newton making it an excellent target for such a study. We find 4 sources which show…

Astrophysics · Physics 2008-11-26 Gavin Ramsay , Louise Harra , Hilary Kay

The examination of two 2010 Chandra ACIS exposures of the Circinus galaxy resulted in the discovery of two pulsators: CXO J141430.1-651621 and CXOU J141332.9-651756. We also detected 26-ks pulsations in CG X-1, consistently with previous…

High Energy Astrophysical Phenomena · Physics 2016-08-08 P. Esposito , G. L. Israel , D. Milisavljevic , M. Mapelli , L. Zampieri , L. Sidoli , G. Fabbiano , G. A. Rodríguez Castillo

We review the main properties, demographics and applications of binary and millisecond radio pulsars. Our knowledge of these exciting objects has greatly increased in recent years, mainly due to successful surveys which have brought the…

Astrophysics · Physics 2016-10-19 D. R. Lorimer

We report the discovery of a bright transient X-ray source, CXOU J132518.2-430304, towards Centaurus A (Cen A) using six new Chandra X-Ray Observatory observations in 2007 March--May. Between 2003 and 2007, its flux has increased by a…

The temporal heating and subsequent cooling of the crusts of transiently accreting neutron stars carries unique information about their structure and a variety of nuclear reaction processes. We report on a new Chandra Director's…

High Energy Astrophysical Phenomena · Physics 2015-05-28 N. Degenaar , E. F. Brown , R. Wijnands