Populations of X-Ray Sources in Galaxies

By G. Fabbiano. 2006

252 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/588ee146014479543c199a468db2eacdf219a3d2

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In Astronomy and Astrophysics

1. D. M. Alexander
2. P. Hopkins
3. L. Hernquist
4. W. N. Brandt
5. R. Hickox
6. Mara Salvato
7. A. Koekemoer
8. P. Capak

In Nuclear and High Energy Physics

1. D. M. Alexander
2. W. N. Brandt
3. G. Hasinger
4. R. Hickox
5. A. Comastri
6. T. Miyaji
7. P. Hopkins
8. Luis C. Ho

Citations in the corpus

• THE CHANDRA COSMOS SURVEY. I. OVERVIEW AND POINT SOURCE CATALOG (2009, background): “Thus close mergers can be resolved, and nuclear sources distinguished from off-nuclear sources in galaxies (Ultra-luminous X-ray Sources, ULXs, Fabbiano 2006, Lehmer et al. 2006, Mainieri et al. 2009, in preparation).”
• x-cigale: fitting AGN/galaxy SEDs from X-ray to infrared (2020, methodology): “In our test fitting in §3, we set Γ to 1.56 and 2.0 for LMXB and HMXB, respectively (e.g. Fabbiano 2006; Sazonov & Khabibullin 2017).”
• REVISITING WITH CHANDRA THE SCALING RELATIONS OF THE X-RAY EMISSION COMPONENTS (BINARIES, NUCLEI, AND HOT GAS) OF EARLY-TYPE GALAXIES (2010, background): “…and sensitivity of the Chandra X-ray Observatory, we have been able for 1 Also at Department of Natural Sciences, Clayton State University, Morrow, GA 30260, USA. the first time to resolve individual point-like sources, such as LMXBs and faint nuclei, in these galaxies (see Fabbiano 2006).”
• Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests (2009, background): “The capture of stars has been put forward as an explanation for ultra-luminous X-ray sources (see e.g. Fabbiano 2006, for a review).”
• A CHANDRA PERSPECTIVE ON GALAXY-WIDE X-RAY BINARY EMISSION AND ITS CORRELATION WITH STAR FORMATION RATE AND STELLAR MASS: NEW RESULTS FROM LUMINOUS INFRARED GALAXIES (2010, background): “…PA 16802, USA In normal star-forming galaxies (i.e., those that are not dominated by luminous active galactic nuclei [AGNs]), X-ray emission originates from X-ray binaries, supernovae, supernova remnants, hot (≈0.2–1 keV) interstellar gas, and O-stars (see, e.g., Fabbiano 1989, 2006 for reviews).”
• Nuclear Activity in Nearby Galaxies (2008, background): “The nucleus, if present, is often encircled by other point sources, mostly XRBs (Fabbiano 2006).”
• STRUCTURE AND FORMATION OF ELLIPTICAL AND SPHEROIDAL GALAXIES (2008, background): “The discrete source contribution toLX is proportional to LB (Fabbiano 2006).”
• X-ray emission from star-forming galaxies – I. High-mass X-ray binaries (2011, background): “Indeed, X-ray output of a normal gas-poor galaxy is dominated by the collective emission of its X-ray binary (XRB) population (see review by Fabbiano 2006).”
• Active galactic nuclei: what’s in a name? (2017, background): “The dominant host-galaxy phenomenon at X-ray energies is commonly referred to as X-ray binaries (see Fabbiano 2006 and Remillard and McClintock 2006 for reviews).”
• The Coincidence of Nuclear Star Clusters and Active Galactic Nuclei (2008, background): “For the higher resolution Chandra and XMM observations, which are localized to be coincident with the NC (see Table 4), the sources with low X-ray luminosities overlap with those expected for X-ray binaries (Fabbiano 2006).”