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Related papers: A Chandra Study of the Circinus Galaxy Point-Sourc…

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We present the source catalog of a new Chandra ACIS-I observation of NGC 300 obtained as part of the Chandra Local Volume Survey. Our 63 ks exposure covers ~88% of the D25 isophote (R~6.3 kpc) and yields a catalog of 95 X-ray point sources…

High quality 4500-6800 A spectropolarimetric observations of the Circinus galaxy are reported. These show polarized and relatively broad (FWHM~3300 km/s) Halpha (as well as marginal Hbeta) arising from a <3" (<60 pc) region centered on the…

Astrophysics · Physics 2007-05-23 E. Oliva , A. Marconi , A. Cimatti , S. di Serego Alighieri

We examine the X-ray spectra and variability of the sample of X-ray sources with L_X = 10^{31}-10^{33} erg s^{-1} identified within the inner 9' of the Galaxy. Very few of the sources exhibit intra-day or inter-month variations. We find…

We have spatially and spectrally resolved the sources of X-ray emission from the X-ray faint S0 galaxy NGC 1553 using an observation from the Chandra X-ray Observatory. The majority (70%) of the emission in the 0.3 - 10.0 keV band is…

Astrophysics · Physics 2009-10-31 E. L. Blanton , C. L. Sarazin , J. A. Irwin

We present the result of the Chandra high-resolution observation of the Seyfert~2 galaxy NGC 7590. This object was reported to show no X-ray absorption in the low-spatial resolution ASCA data. The XMM observations show that the X-ray…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Xinwen Shu , Junxian Wang , Teng Liu , Wei Zheng

The advanced capabilities of the Chandra and XMM-Newton observatories mean that, for the first time, the detailed study of the brightest point-like X-ray sources in nearby galaxies outside of the local group is a realistic aim. Here, we…

Astrophysics · Physics 2007-05-23 T. P. Roberts , M. R. Goad , M. J. Ward , R. S. Warwick , P. Lira

As part of our campaign to determine the nature of the various source populations of the low-luminosity globular cluster X-ray sources, we have obtained a Chandra X-ray Observatory ACIS-S3 image of the globular cluster NGC 6440. We detect…

(Abridged) We present the LogN-LogS and spatial distributions of X-ray point sources in seven Galactic Bulge (GB) fields within 4 deg from the Galactic Center (GC). We compare the properties of 1159 X-ray point sources discovered in our…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Jaesub Hong , Maureen van den Berg , Jonathan E. Grindlay , Silas Laycock

We have obtained three epochs of Chandra ACIS-I observations (totaling $\sim$184 ks) of the nearby spiral galaxy NGC~300 to study the logN-logS distributions of its X-ray point source population down to $\sim$2$\times$10$^{-15}$ erg…

High Energy Astrophysical Phenomena · Physics 2017-01-18 Breanna Binder , Jacob Gross , Benjamin F. Williams , Michael Eracleous , Terrance J. Gaetz , Paul P. Plucinsky , Evan D. Skillman

We report the identification of a possible optical counterpart to the super-Eddington X-ray source NGC 5204 X-1. New Chandra data shows that the X-ray source is point-like, with a luminosity of 5.2 x 10^39 erg/s (0.5 - 8 keV). It displays…

Astrophysics · Physics 2009-11-06 T. P. Roberts , M. R. Goad , M. J. Ward , R. S. Warwick , P. T. O'Brien , P. Lira , A. D. P. Hands

We present a detailed X-ray spectral analysis of the Circinus Galaxy using archival data obtained with the ASCA satellite. The spectrum shows numerous emission lines in the soft X-ray band from highly ionized ions, as well as Compton…

Astrophysics · Physics 2009-10-31 Masao Sako , Steven M. Kahn , Frits Paerels , Duane A. Liedahl

We report the results of a programme of dual-epoch Chandra ACIS-S observations of five ultraluminous X-ray sources (ULXs) in nearby spiral galaxies. All five ULXs are detected as unresolved, point-like X-ray sources by Chandra, though two…

Astrophysics · Physics 2009-11-10 T. P. Roberts , R. S. Warwick , M. J. Ward , M. R. Goad

The aim of this work is to identify the so far unknown low mass stellar population of the ~2Myr old Cygnus OB2 region, and to investigate the X-ray and near-IR stellar properties of its members. We analyzed a 97.7 ksec Chandra ACIS-I…

Astrophysics · Physics 2009-11-11 J. F. Albacete Colombo , E. Flaccomio , G. Micela , F. Damiani , S. Sciortino

We report a study of X-ray-irradiated gas in the central ~100 pc of the Circinus galaxy, hosting a Compton-thick active galactic nucleus (AGN), at 10-pc resolution using Chandra and ALMA. Based on ~200 ksec Chandra/ACIS-S data, we created…

Astrophysics of Galaxies · Physics 2019-07-10 Taiki Kawamuro , Takuma Izumi , Masatoshi Imanishi

We report the detection of six discrete, low-luminosity (Lx < 10^33 erg/s) X-ray sources, located within 12 arcsec of the center of the collapsed-core globular cluster M30 (NGC 7099), and a total of 13 sources within the half-mass radius,…

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…

The emission-line dwarf galaxy NGC 3413 is known to host a bright X-ray source near its optical center. The 0.3-10 keV luminosity of this source is estimated to be approximately 10$^{39}$ erg$s^{-1}$ potentially qualifying it as an…

High Energy Astrophysical Phenomena · Physics 2018-10-17 E. Sonbas , K. S. Dhuga , E. Göğüş

We present the properties of the discrete X-ray sources detected in our monitoring program of the globular cluster (GC) rich elliptical galaxy, NGC 4278, observed with Chandra ACIS-S in six separate pointings, resulting in a co-added…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-13 N. J. Brassington , G. Fabbiano , D. -W. Kim , A. Zezas , S. Zepf , A. Kundu , L. Angelini , R. L. Davies , J. Gallagher , V. Kalogera , T. Fragos , A. R. King , S. Pellegrini , G. Trinchieri

Circinus X-1 (Cir X-1) is a neutron star binary with an elliptical orbit of 16.6~days. The source is unique for its extreme youth, providing a key to understanding early binary evolution. However, its X-ray variability is too complex to…

High Energy Astrophysical Phenomena · Physics 2023-11-15 Mayu Tominaga , Masahiro Tsujimoto , Ken Ebisawa , Teruaki Enoto , Kimitake Hayasaki