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Intermediate polars are a class of cataclysmic variables in which a white dwarf accretes material from a companion star. The intermediate polar nature confirmation usually derives from the detection of two periods in both $X$-ray and…

High Energy Astrophysical Phenomena · Physics 2026-01-21 A. A. Nucita , S. M. Lezzi , F. De Paolis , Strafella , D. Licchelli , A. Franco , M. Maiorano

An X-ray compact source was discovered with Chandra in a supernova remnant (SNR) N23, located in the Large Magellanic Cloud. The compact source (CXOU J050552.3-680141) is seen in only the hard band (> 2 keV) image of N23, while the soft…

Astrophysics · Physics 2008-11-26 Asami Hayato , Aya Bamba , Toru Tamagawa , Kiyoshi Kawabata

We present a Chandra X-ray Observatory ACIS-S variability, spectroscopy, and imaging study of the peculiar binary containing the millisecond pulsar J1023+0038. The X-ray emission from the system exhibits highly significant (12.5 sigma)…

We present the results of a Suzaku study of a bright point-like source in the 6.7 keV intensity map of the Galactic center region. We detected an intense FeXXV 6.7 keV line with an equivalent width of ~1 keV as well as emission lines of…

This paper reports on an analysis of two Chandra X-ray observations of the young magnetic B star rho Ophiuchus S1. X-ray emission from the star was detected in both observations. The average flux was almost the same in both, but during each…

Astrophysics · Physics 2015-06-24 Kenji Hamaguchi , Michael F. Corcoran , Kensuke Imanishi

We present timing and spectral analysis of a sample of seven hard X-ray selected Cataclysmic Variable candidates based on simultaneous X-ray and optical observations collected with XMM-Newton , complemented with Swift/BAT and INTEGRAL/IBIS…

High Energy Astrophysical Phenomena · Physics 2017-08-02 F. Bernardini , D. de Martino , K. Mukai , D. M. Russell , M. Falanga , N. Masetti , C. Ferrigno , G. Israel

The ISOGAL mid-infrared survey of areas close to the Galactic Plane aims to determine their stellar content and its possible bearing on the history of the Galaxy. The NGC6522 and Sgr I Baade's Windows of low obscuration towards the inner…

We have observed the eclipsing low-mass X-ray binary MS1603.6+2600 with Chandra for 7 ksec. The X-ray spectrum is well fit with a single absorbed powerlaw with an index of ~2. We find a clear sinusoidal modulation in the X-ray lightcurve…

Astrophysics · Physics 2009-11-10 P. G. Jonker , M. van der Klis , C. Kouveliotou , M. Mendez , W. H. G. Lewin , T. Belloni

IGR J14257-6117 is an unclassified source in the hard X-ray catalogues. Optical follow-ups suggest it could be a Cataclysmic Variable of the magnetic type. We present the first high S/N X-ray observation performed by \XMM\ at 0.3--10 keV,…

High Energy Astrophysical Phenomena · Physics 2018-05-16 F. Bernardini , D. de Martino , K. Mukai , M. Falanga

We present the first results of the Chandra and optical follow-up observations of hard X-ray sources detected in the ASCA Medium Sensitivity Survey (AMSS). Optical identifications are made for five objects. Three of them show either weak or…

We present the first results of ChaMP X-ray source properties obtained from the initial sample of 62 observations. The data have been uniformly reduced and analyzed with techniques specifically developed for the ChaMP and then validated by…

We report the discovery of X-ray emission from NGC 7027, a prototypical object for the study of the formation and evolution of planetary nebulae (PNs). Observations with the Advanced CCD Imaging Spectrometer (ACIS) aboard the Chandra X-ray…

Astrophysics · Physics 2009-11-06 Joel H. Kastner , Saeqa D. Vrtilek , Noam Soker

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 discovered Fe $K_{\alpha}$ complex emission and pulsation in two highly variable sources (4XMM J174917.7--283329, 4XMM J174954.6--294336). The equivalent widths of 6.4 and 6.7 keV lines of 4XMM J174917.7--283329 are $99^{+84}_{-72}$ and…

High Energy Astrophysical Phenomena · Physics 2023-03-15 Samaresh Mondal , Gabriele Ponti , Frank Haberl , Kaya Mori , Nanda Rea , Mark R. Morris , Sergio Campana , Konstantina Anastasopoulou

We present the results of a 63 ks {\it Chandra} observation of the "supernova impostor" SN 2010da four months after it was first observed on 25 May 2010. We detect an X-ray source at $\sim7\sigma$ confidence coincident with the optical…

High Energy Astrophysical Phenomena · Physics 2015-05-28 B. Binder , B. F. Williams , A. K. H. Kong , T. J. Gaetz , P. P. Plucinsky , J. J. Dalcanton , D. R. Weisz

The field containing the candidate High Mass X-ray Binary IGR J01363+6610 was observed by XMM-Newton on 2009 July 31 for 28 ks. A Be star was previously suggested as the possible counterpart of the INTEGRAL source, and although Chandra,…

High Energy Astrophysical Phenomena · Physics 2015-05-20 John A. Tomsick , Craig Heinke , Jules Halpern , Philip Kaaret , Sylvain Chaty , Jerome Rodriguez , Arash Bodaghee

Polarized diffuse emission observations at 1.4-GHz in a high Galactic latitude area of the northern Celestial hemisphere are presented. The 3.2 X 3.2 deg^2 field, centred at RA = 10h 58m, Dec = +42deg 18' (B1950), has Galactic coordinates…

Astrophysics · Physics 2009-11-13 E. Carretti , S. Poppi , W. Reich , P. Reich , E. Fuerst , G. Bernardi , S. Cortiglioni , C. Sbarra

(Abridged) We have analyzed Chandra LETG and XMM-Newton RGS spectra towards the z=0.177 quasar PG 1116+215, a sightline that is rendered particularly interesting by the HST detection of several OVI and HI broad Lyman-alpha absorption lines…

Cosmology and Nongalactic Astrophysics · Physics 2016-02-17 M. Bonamente , J. Nevalainen , E. Tilton , J. Liivamagi , E. Tempel , P. Heinamaki , T. Fang

We present results from a 47 ks observation of the Andromeda galaxy, M31, using the High-Resolution Camera of the Chandra X-Ray Observatory. We detect 142 point sources spanning three orders of magnitude in luminosity, from $L_X = 2\times…

Astrophysics · Physics 2009-11-07 Philip Kaaret

We present the analysis of serendipitous sources in a deep, 500 ksec, hard X-ray observation of the Coma cluster region with the IBIS instrument onboard INTEGRAL. In addition to the Coma cluster, the final 20-50 keV image contains 12…

Astrophysics · Physics 2009-11-10 R. Krivonos , A. Vikhlinin , E. Churazov , A. Lutovinov , S. Molkov , R. Sunyaev