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Chandra observations of the X-ray faint elliptical galaxy NGC 4697 resolve much of the X-ray emission (61% within one effective radius) into ~80 point sources, of which most are low mass X-ray binaries (LMXBs). These LMXBs provide the bulk…

Astrophysics · Physics 2009-10-31 Craig L. Sarazin , Jimmy A. Irwin , Joel N. Bregman

Presented here are the highlights from the deep Chandra observation of the elliptical galaxy NGC 3379. From the multi-epoch observation of this galaxy, 132 discrete X-ray sources have been detected within the region overlapped by all…

Astrophysics · Physics 2007-12-24 N. J. Brassington

We determine the total enclosed mass profile from 0.7 to 35 kpc in the elliptical galaxy NGC 4636 based on the hot interstellar medium temperature profile measured using the Chandra X-ray Observatory, and other X-ray and optical data. The…

Astrophysics · Physics 2007-05-23 M. Loewenstein , R. Mushotzky

We have used a deep Chandra observation of the central regions of the twin-jet FRI radio galaxy 3C31 to resolve the thermal X-ray emission in the central few kiloparsecs of the host galaxy, NGC 383, where the jets are thought to be…

Astrophysics · Physics 2009-11-07 M. J. Hardcastle , D. M. Worrall , M. Birkinshaw , R. A. Laing , A. H. Bridle

We present 26 point-sources discovered with Chandra within 200" (~20kpc) of the center of the barred supergiant galaxy NGC 1365. The majority of these sources are high-mass X-ray binaries, containing a neutron star or a black hole accreting…

Astrophysics · Physics 2011-02-11 Iskra V. Strateva , Stefanie Komossa

With a Chandra ACIS-S3 observation, we detect 42 X-ray point sources in the elliptical galaxy NGC 720, including a possible central source. Most of these sources will be low-mass X-ray binaries (LMXBs), and 12 are located within 2" of…

Astrophysics · Physics 2009-11-07 Tesla E. Jeltema , Claude R. Canizares , David A. Buote , Gordon P. Garmire

Deep Chandra observations (53 ks, ACIS-S3) of NGC 3077, a starburst dwarf galaxy in the M 81 triplet, resolve the X-ray emission from several supershells. The emission is brightest in the cavities defined by expanding shells detected…

Astrophysics · Physics 2009-11-07 Juergen Ott , Crystal L. Martin , Fabian Walter

We report the discovery of a faint (L_x ~ 4 10^37 erg/s, 0.5-2 keV), out-flowing gaseous hot interstellar medium (ISM) in NGC 3379. This represents the lowest X-ray luminosity ever measured from a hot phase of the ISM in a nearby early type…

We present Chandra and XMM-Newton X-ray data of NGC5253, a local starbursting dwarf elliptical galaxy, in the early stages of a starburst episode. Contributions to the X-ray emission come from discrete point sources and extended diffuse…

Astrophysics · Physics 2009-11-10 Lesley K. Summers , Ian R. Stevens , David K. Strickland , Timothy M. Heckman

We present a detailed analysis of high-resolution Chandra observations of the merger system NGC3256, the most IR luminous galaxy in the nearby universe. The X-ray data show that several discrete sources embedded in complex diffuse emission…

Astrophysics · Physics 2009-11-07 P. Lira , M. Ward , A. Zezas , A. Alonso-Herrero , S. Ueno

Using high resolution Chandra data, we report the presence of a weak X-ray point source coincident with the nucleus of NGC 4178, a late-type bulgeless disk galaxy known to have high ionization mid-infrared (mid-IR) lines typically…

Astrophysics of Galaxies · Physics 2015-06-05 Nathan Secrest , Shobita Satyapal , Mario Gliozzi , C. C. Cheung , Anil Seth , Torsten Boeker

By studying the optical brightness surface density of the globular cluster NGC 6388, it has been recently proposed that it harbors a central intermediate-mass black hole with mass $\simeq 5.7\times 10^3$ M$_{\odot}$. We expect that the…

Astrophysics · Physics 2007-12-17 A. A. Nucita , F. De Paolis , G. Ingrosso , S. Carpano , M. Guainazzi

We report the detection of hard X-ray emission components in the spectra of six nearby, giant elliptical galaxies observed with the ASCA satellite. The systems studied, which exhibit strong dynamical evidence for supermassive black holes in…

Astrophysics · Physics 2009-10-31 S. W. Allen , T. Di Matteo , A. C. Fabian

We present a Chandra ACIS-S observation of the nearby bulge-dominated Sa galaxy NGC1291. The X-ray emission from the bulge resembles the X-ray emission from a sub-class of elliptical and S0 galaxies with low L_X/L_B luminosity ratios. The…

Astrophysics · Physics 2009-11-06 Jimmy A. Irwin , Craig L. Sarazin , Joel N. Bregman

We report results of an 18 ks exposure with the ACIS instrument on Chandra of the powerful z = 0.62 radio galaxy 3C 220.1. The X-ray emission separates into cluster gas of emission-weighted kT ~ 5 keV and 0.7-12 keV luminosity (to a radius…

Astrophysics · Physics 2009-11-06 D. M. Worrall , M. Birkinshaw , M. J. Hardcastle , C. R. Lawrence

In a 52 ks-long Chandra ACIS-S observation of the nearby starburst galaxy NGC 3628, obtained to study the starburst-driven outflow from this galaxy, we have detected a very luminous (L_X = 1.1e40 erg/s in the 0.3-8.0 keV energy band) point…

We report Chandra observations of the Scd galaxy NGC 2139, which is known to host a recently formed (10^7.6 yrs) nuclear star cluster. The star cluster is undetected in X-rays, with an upper bound on 0.5-7 keV luminosity of L_X < 7.1 x…

Astrophysics of Galaxies · Physics 2015-06-05 Joseph C. Shields , Torsten Boeker , Luis C. Ho , Hans-Walter Rix , Roeland P. van der Marel , C. Jakob Walcher

We present CHANDRA X-ray data of the nearby Magellanic Irregular dwarf starburst galaxy NGC4449. Contributions to the X-ray emission come from discrete point sources and extended diffuse emission. The extended emission has a complex…

Astrophysics · Physics 2009-11-07 Lesley K. Summers , Ian R. Stevens , David K. Strickland , Timothy M. Heckman

We present results from Planetary Nebula Spectrograph (PN.S) observations of the elliptical galaxy NGC 3379 and a description of the data reduction pipeline. We detected 214 planetary nebulae of which 191 are ascribed to NGC 3379, and 23 to…

We report results of a Chandra observation of the X-ray luminous star-forming galaxy Arp299 (NGC3690/IC694). We detect 18 discrete X-ray sources with luminosities above ~10^39 erg\s (0.5-8.0 keV band), which contribute ~40% of the total…

Astrophysics · Physics 2009-11-10 A. Zezas , M. J. Ward , S. S. Murray