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Related papers: X-rays from the barred galaxy NGC 4303

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XMM-Newton EPIC observations reveal the population of X-ray sources of the bright Local Group spiral galaxy M 31, a low-star-formation-rate galaxy like the Milky Way, down to a 0.2-4.5 keV luminosity of 4.4E34 erg/s. With the help of X-ray…

Astrophysics · Physics 2007-05-23 W. Pietsch

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

We present results from the cross-correlation of the spectroscopic atlas of Ho etal (1995) with the ROSAT All-Sky Survey Bright Source Catalogue, in an attempt to understand the X-ray emission mechanisms in nearby galaxies. The resulting…

Astrophysics · Physics 2016-08-30 A. L. Zezas , I. Georgantopoulos , M. J. Ward

The NGC 5903 galaxy group is a nearby (~30 Mpc) system of ~30 members, dominated by the giant ellipticals NGC 5903 and NGC 5898. The group contains two unusual structures, a ~110 kpc long HI filament crossing NGC 5903, and a ~75 kpc wide…

We analyzed a deep Chandra observation of M84, a bright elliptical galaxy in the core of the Virgo cluster. We find that the spatial distribution of the soft X-ray emission is defined by the radio structure of the galaxy. In particular we…

Astrophysics · Physics 2009-10-31 A. Finoguenov , C. Jones

We present high spatial resolution X-ray Chandra HRC and HST WFPC2 Halpha observations of the prototypical infrared luminous galaxy NGC6240. The central region of this system shows a remarkably complex morphology, with filaments and loops…

Astrophysics · Physics 2009-11-07 P. Lira , M. J. Ward , A. Zezas , S. S. Murray

Here we present new optical data from the Hubble Space Telescope of the NGC 253 central region, which reveal numerous discrete sources in a ring--like structure. This is combined with data at infrared, millimeter, radio and X-ray…

(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

We present new Spitzer Space Telescope data on the nearby, low-metallicity starburst galaxy NGC 5253, from the Infrared Array Camera IRAC and the Infrared Spectrograph IRS. The mid-IR luminosity profile of NGC 5253 is clearly dominated by…

Astrophysics · Physics 2009-11-11 P. Beirao , B. R. Brandl , D. Devost , J. D. Smith , L. Hao , J. R. Houck

We report on the first deeper X-ray broad-band observation of the hot spot galaxy NGC 2903 obtained with XMM-Newton. X-ray imaging and spectra of the spiral barred galaxy were obtained from XMM-Newton archival data to study its X-ray…

High Energy Astrophysical Phenomena · Physics 2015-05-20 D. Perez-Ramirez , M. D. Caballero-Garcia , J. Ebrero , S. Leon

We present ASCA X-ray results on two S0 galaxies, NGC 3065 and NGC 4203. In both galaxies, we detected hard X-ray emission from a point-like source at the nucleus. Single power law model having a photon index of 1.8 well described the…

We present Chandra ACIS-I and ACIS-S observations ($\sim$200 ks in total) of the X-ray luminous elliptical galaxy NGC 4636, located in the outskirts of the Virgo cluster. A soft band (0.5-2 keV) image shows the presence of a bright core in…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 A. Baldi , W. Forman , C. Jones , R. Kraft , P. Nulsen , E. Churazov , L. David , S. Giacintucci

The nearby barred spiral galaxy NGC 1672 shows dramatic starburst activity and may also host a Seyfert 2 nucleus. We present new X-ray observations that set constraints on starburst and Seyfert activity in NGC 1672. Two ROSAT HRI exposures,…

Astrophysics · Physics 2009-10-31 P. J. de Naray , W. N. Brandt , J. P. Halpern , K. Iwasawa

We present the Chandra discovery of soft diffuse X-ray emission in NGC 4151 (L[0.5-2keV]~10^{39} erg s$^{-1}$), extending ~2 kpc from the active nucleus and filling in the cavity of the HI material. The best fit to the X-ray spectrum…

Galaxy formation models predict that local galaxies are surrounded by hot X-ray-emitting halos, which are technically difficult to detect due to their extended and low surface brightness nature. Previous X-ray studies have mostly focused on…

Astrophysics of Galaxies · Physics 2025-03-14 Lin He , Zhiyuan Li , Meicun Hou , Min Du , Taotao Fang , Wei Cui

We present a systematic study of the putative hot gas corona around late-type galaxies (LTGs) residing in the Virgo cluster, based on archival Chandra observations. Our sample consists of 21 nearly edge-on galaxies representing a star…

Astrophysics of Galaxies · Physics 2023-12-08 Meicun Hou , Lin He , Zhensong Hu , Zhiyuan Li , Christine Jones , William Forman , Yuanyuan Su , Jing Wang , Luis C. Ho

NGC 1232 is a face-on spiral galaxy and a great laboratory for the study of star-formation due to its proximity. We obtained high spatial resolution H{\alpha} images of this galaxy, with adaptive optics, using the SAM instrument at the SOAR…

Astrophysics of Galaxies · Physics 2018-05-28 Alexandre Araújo de Souza , Lucimara P. Martins , Alberto Rodríguez-Ardila , Luciano Fraga

We found several extranuclear (r >~ 3") X-ray nebulae within 40" (6.3 kpc at 32.5 Mpc) of the nucleus of the Seyfert galaxy NGC 2992. The net X-ray luminosity from the extranuclear sources is ~2-3 E39 erg/s (0.3-8.0 keV). The X-ray core…

We utilize the complimentary capabilities of XMM-Newton and Chandra, to conduct a detailed imaging and spectral study of the nearby galaxy NGC 4945 focussing on its nucleus and immediate surroundings (within ~1 kpc of the nucleus). A…

Astrophysics · Physics 2016-08-30 N. J. Schurch , T. P. Roberts , R. S. Warwick

VLA and Parkes 64 m radiotelescope 21-cm observations of the starburst dwarf galaxy NGC 5253 reveal a multi-component non-axisymmetric HI distribution. The component associated with the stellar body shows evidence for a small amount of…

Astrophysics · Physics 2009-11-13 Henry A. Kobulnicky , Evan. D. Skillman