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We present a Chandra observation of Abell 2052, a cooling flow cluster with a central cD that hosts the complex radio source 3C 317. The data reveal ``holes'' in the X-ray emission that are coincident with the radio lobes. The holes are…

Astrophysics · Physics 2009-11-06 Elizabeth L. Blanton , Craig L. Sarazin , Brian R. McNamara , Michael W. Wise

(Abridged) We observed the X-ray bright E3 galaxy NGC 1600 and nearby group members with the Chandra X-ray Observatory ACIS S3. Unresolved emission dominates the observation; however, we resolved some emission into 71 sources, most of which…

Astrophysics · Physics 2009-11-10 Gregory R. Sivakoff , Craig L. Sarazin , Jeffrey L. Carlin

Using the Chandra ACIS-I instruments, we have carried out the deepest X-ray observation on a typical Galactic plane region at l 28.5 deg, where no discrete X-ray sources have been known previously. We have detected, as well as strong…

Astrophysics · Physics 2016-11-03 K. Ebisawa , A. Bamba , H. Kaneda , Y. Maeda , A. Paizis , G. Sato , S. Yamauchi

We use a Chandra X-ray observation of the gravitationally lensed system MGB2016+112 at z=3.273 to elucidate presence of at least two X-ray sources. We find that these sources are consistent with the VLBI components measured by…

High Energy Astrophysical Phenomena · Physics 2021-08-25 Daniel Schwartz , Cristiana Spingola , Anna Barnacka

We analyse a Chandra observation of the rich globular cluster NGC 362, finding 33 X-ray sources within 1' (1.2 half-mass radii) of the cluster center. Spectral analysis of the brightest source (X1) shows blackbody-like emission, indicating…

High Energy Astrophysical Phenomena · Physics 2024-03-26 Gourav Kumawat , Craig O. Heinke , Haldan N. Cohn , Phyllis M. Lugger

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

Chandra images of galaxy clusters have revealed a wealth of structure unseen by previous generations of low resolution X-ray observatories. In the cores of clusters, bright, irregular X-ray emission is now routinely seen within central…

Astrophysics · Physics 2007-05-23 B. R. McNamara

An observation of the radio galaxy 3C295 during the calibration phase of the Chandra X-ray Observatory reveals X-ray emission from the core of the galaxy, from each of the two prominent radio hotspots, and from the previously known cluster…

We present a detailed study of the X-ray, optical and radio emission from the jet, lobes and core of the quasar PKS 2101-490 as revealed by new Chandra, HST and ATCA images. We extract the radio to X-ray spectral energy distributions from…

Observations with BeppoSAX, RXTE and Chandra suggest that many of the bright X-ray sources in globular clusters have ultrashort binary periods. This is remarkable as such systems are not easily formed. With accurate optical astrometry of…

Astrophysics · Physics 2009-11-10 Frank Verbunt

We present Chandra observations of a small sample of nearby classical double radio galaxies which have more than one radio hotspot in at least one of their lobes. The X-ray emission from the hotspots of these comparatively low-power objects…

Astrophysics · Physics 2009-11-13 M. J. Hardcastle , J. H. Croston , R. P. Kraft

We report detailed studies of the X-ray emission from the kpc scale jet in the nearest active galaxy, Cen A. 41 compact sources were found within the jet, 13 of which were newly identified. We construct the luminosity function for the…

The physical nature of ultraluminous x-ray sources is uncertain. Stellar mass black holes with beamed radiation and intermediate mass black holes with isotropic radiation are two plausible explanations. We discovered radio emission from an…

Astrophysics · Physics 2009-11-07 Philip Kaaret , Stephane Corbel , Andrea H. Prestwich , Andreas Zezas

This paper presents the analysis of Chandra X-ray snapshot observations of a subsample of the extragalactic sources listed in the revised Third Cambridge radio catalog (3CR), previously lacking X-ray observations and thus observed during…

Seyfert galaxies and quasars were first discovered through optical and radio techniques, but in recent years high-energy emission, that can penetrate central gas and dust, has become essentially the defining characteristic of an AGN. AGNs…

Astrophysics · Physics 2007-05-23 D. M. Worrall

I review our recent Chandra surveys of the center region of the Milky Way and other nearby edge-on galaxies. Our Galactic center survey provides an unprecedented high-resolution, broad-band X-ray panorama of a 0.8x2 square degree swath…

Astrophysics · Physics 2007-05-23 Q. Daniel Wang

We present a detailed case study of the diffuse X-ray and H-alpha emission in the halo of NGC 253, a nearby edge-on starburst galaxy driving a galactic superwind. The arcsecond spatial resolution of the Chandra ACIS instrument allows us to…

Astrophysics · Physics 2009-11-07 D. K. Strickland , T. M. Heckman , K. A. Weaver , C. G. Hoopes , M. Dahlem

We present Chandra observations of 18 spectroscopically selected quasars, already known to be X-ray weak from previous ROSAT observations. All the sources but one are detected by Chandra, and spectral analysis suggests that most of them are…

Astrophysics · Physics 2009-11-07 G. Risaliti , M. Elvis , R. Gilli , M. Salvati

We report on new multi-frequency Very Large Array (VLA) radio observations and Chandra X-ray observations of a radio-loud quasar with a ~300 kpc long jet, PKS 1127-145, during a flaring event detected in $\gamma$-rays by the Fermi Large…

High Energy Astrophysical Phenomena · Physics 2024-07-24 M. Orienti , A. Siemiginowska , F. D'Ammando , G. Migliori

We report on the direct observation of an extended X-ray jet in the $z$=6.1 radio-loud Active Galactic Nucleus PSO J030947.49+271757.31 from a deep Chandra X-ray observation (128 ksec). This detection represents the most distant kpc…

High Energy Astrophysical Phenomena · Physics 2022-03-14 L. Ighina , A. Moretti , F. Tavecchio , A. Caccianiga , S. Belladitta , D. Dallacasa , R. Della Ceca , T. Sbarrato , C. Spingola
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