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We present the XMM-Newton observations obtained during four revolutions in Spring and Summer 2004 of CXOGC J174540.0-290031, a moderately bright transient X-ray source, located at only 2.9" from SgrA*. We report the discovery of sharp and…

Astrophysics · Physics 2009-11-11 D. Porquet , N. Grosso , G. Belanger , A. Goldwurm , F. Yusef-Zadeh , R. S. Warwick , P. Predehl

We report the results from a Chandra TOO observation of the low-luminosity Narrow Line Seyfert 1 galaxy NGC 4051, obtained during a 6-week duration low-flux state in 2001 February. During the Chandra observation, the 2-10 keV source flux…

Astrophysics · Physics 2009-11-07 P. Uttley , A. Fruscione , I. McHardy , G. Lamer

We discovered eclipses and dips in two luminous (and highly variable) X-ray sources in M\,51. One (CXOM51 J132943.3$+$471135) is an ultraluminous supersoft source, with a thermal spectrum at a temperature of about 0.1 keV and characteristic…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Song Wang , Roberto Soria , Ryan Urquhart , Jifeng Liu

Details of simultaneous photometric and spectroscopic observations of the optical counterpart of the `supersoft' X-ray source 1E 0035.4-7230 (SMC 13) are presented. Although the spectrum is dominated by emission lines of He II, the Balmer…

Astrophysics · Physics 2007-05-23 David Crampton , J. B. Hutchings , A. P. Cowley , P. C. Schmidtke

A comparison is made between the properties of CAL 83, CAL 87, RX J0513.9-6951, 1E 0035.4-7230 (SMC 13), RX J0019.8+2156, and RX J0925.7-4758, all supersoft X-ray binaries. Spectra with the same resolution and wavelength coverage of these…

Astrophysics · Physics 2016-08-30 A. P. Cowley , P. C. Schmidtke , D. Crampton , J. B. Hutchings

We present an analysis of the first observation of the iconic High Mass X-ray Binary \so with the \chandra High Energy Transmission Gratings during an X-ray eclipse. The goal of the observation was to study the structure/physical conditions…

High Energy Astrophysical Phenomena · Physics 2021-01-06 M. Martínez-Chicharro , V. Grinberg , J. M. Torrejón , N. Schulz , L. Oskinova , M. Nowak , F. Fürst , N. Hell , R. Hainich

We present high-resolution X-ray spectroscopy of GRB 020405 obtained with the Low Energy Transmission Grating Spectrometer (LETGS) on board the Chandra X-ray Observatory starting 1.68 days after the burst. The spectrum appears featureless,…

Astrophysics · Physics 2009-11-07 N. Mirabal , F. Paerels , J. P. Halpern

The bright eclipsing and bursting low-mass X-ray binary EXO 0748-676 has been observed at several occasions by XMM-Newton during the initial calibration and performance verification (CAL/PV) phase. We present here the results obtained from…

Astrophysics · Physics 2009-10-31 J. M. Bonnet-Bidaud , F. Haberl , P. Ferrando , P. J. Bennie , E. Kendziorra

This catalog comprises an up-to-date list of luminous (>10^36 erg/s) supersoft X-ray sources. We include in this catalog accreting binary sources of high luminosity which are thought to be in a state of (steady or recurrent) hydrogen…

Astrophysics · Physics 2015-06-24 J. Greiner

The eclipsing X-ray binary M33 X-7 was in the field of view during several observations of our XMM-Newton M33 survey and in the archival Chanfdra observation 1730 which cover a large part of the 3.45 d orbital period. We detect emission of…

Astrophysics · Physics 2009-11-10 W. Pietsch , B. J. Mochejska , Z. Misanovic , F. Haberl , M. Ehle , G. Trinchieri

We present Chandra and XMM-Newton observations of the composite star-forming/Seyfert galaxy IRAS20051-1117. The X-ray imaging and spectral properties reveal the presence of an active nucleus. The Chandra image shows a strong nuclear point…

Astrophysics · Physics 2009-11-10 I. Georgantopoulos , I. Papadakis , A. Zezas , M. J. Ward

We present a non-LTE model atmosphere analysis of Chandra HRC-S/LETG and XMM-Newton RGS spectroscopy of the prototypical supersoft source CAL 83 in the Large Magellanic Cloud. Taken with a 16-month interval, the Chandra and XMM-Newton…

We present optical photometry of the eclipsing supersoft source, CAL87. These observations comprise long term data accumulated as a by-product of the MACHO Project, and high speed white light photometry of a single eclipse. We (i) derive an…

Astrophysics · Physics 2015-06-24 C. Alcock

The analysis of hard X-ray INTEGRAL observations (2003-2008) of superaccreting galactic microquasar SS433 at precessional phases of the source with the maximum disk opening angle is carried out. It is found that the shape and width of the…

High Energy Astrophysical Phenomena · Physics 2009-04-23 A. M. Cherepashchuk , R. A. Sunyaev , K. A. Postnov , E. A. Antokhina , S. V. Molkov

We report on the first near-simultaneous X-ray and optical observations of RX J0806.3+1527. The source is believed to be a 321s orbital period ultra-compact binary system hosting an X-ray emitting white dwarf. Data were obtained with…

We present X-ray observations of nine Weak-Line Radio Galaxies (WLRGs), optically classified as confirmed or possible Low Ionization Nuclear Emission-line Regions (LINERs). The data were taken from the Chandra, XMM, and BeppoSax archives.…

Astrophysics · Physics 2009-11-10 Alexander S. Rinn , Rita M. Sambruna , Mario Gliozzi

A Chandra ACIS-S imaging observation of the nearby galaxy M81 (NGC 3031) reveals 9 luminous soft X-ray sources. The local environments, X-ray spectral properties, and X-ray light curves of the sources are presented and discussed in the…

Astrophysics · Physics 2009-11-07 Douglas Swartz , Kajal Ghosh , Valery Suleimanov , Allyn Tennant , Kinwah Wu

We observed the accreting white dwarf 1E1339.8+2837 (1E1339) in the globular cluster M3 in Nov. 2003, May 2004 and Jan. 2005, using the Chandra ACIS-S detector. The source was observed in 1992 to possess traits of a supersoft X-ray source…

High Energy Astrophysical Phenomena · Physics 2015-05-27 W. S. Stacey , C. O. Heinke , R. F. Elsner , P. D. Edmonds , M. C. Weisskopf , J. E. Grindlay

We present the X-ray properties of a sample of 17 radio sources observed with the Chandra X-ray Observatory as part of a project aimed at studying the X-ray emission from their radio jets. In this paper, we concentrate on the X-ray…

We have monitored the Seyfert galaxy NGC 3227 with the Rossi X-ray Timing Explorer (RXTE) since January 1999. During late 2000 and early 2001 we observed an unusual hardening of the 2-10 keV X-ray spectrum which lasted several months. The…

Astrophysics · Physics 2009-11-07 G. Lamer , P. Uttley , I. M. McHardy