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(NuSTARNuSTAR) hard X-ray survey of the Galactic Center region. II. X-ray point sources

Journal Article · · Astrophysical Journal
;  [1]; ; ; ; ;  [2];  [3];  [4];  [5];  [6]; ; ;  [7];  [8];  [9];  [10];  [11];  [12];  [13] more »; « less
  1. Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138 (United States)
  2. Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027 (United States)
  3. Astronomy Department, University of California, Berkeley CA 94720 (United States)
  4. Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow (Russian Federation)
  5. Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Catolica de Chile, 306, Santiago 22 (Chile)
  6. Haverford College, 370 Lancaster Avenue, KINSC L109, Haverford, PA 19041 (United States)
  7. Space Sciences Laboratory, University of California, Berkeley, CA 94720 (United States)
  8. Georgia College, 231 W. Hancock St., Milledgeville, GA 31061 (United States)
  9. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States)
  10. Department of Physics, Durham University, Durham DH1 3LE (United Kingdom)
  11. Standford National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94025 (United States)
  12. Kavli Institute for Astrophysics and Space Research, Massachusets Institute of Technology, Cambridge, MA 02139 (United States)
  13. Université de Toulouse, UPS-OMP, IRAP, Toulouse (France)
We present the first survey results of hard X-ray point sources in the Galactic Center (GC) region by NuSTAR. We have discovered 70 hard (3–79 keV) X-ray point sources in a 0.6 deg{sup 2} region around Sgr A* with a total exposure of 1.7 Ms, and 7 sources in the Sgr B2 field with 300 ks. We identify clear Chandra counterparts for 58 NuSTAR sources and assign candidate counterparts for the remaining 19. The NuSTAR survey reaches X-ray luminosities of ∼4× and ∼8 × 10{sup 32} erg s{sup −1} at the GC (8 kpc) in the 3–10 and 10–40 keV bands, respectively. The source list includes three persistent luminous X-ray binaries (XBs) and the likely run-away pulsar called the Cannonball. New source-detection significance maps reveal a cluster of hard (>10 keV) X-ray sources near the Sgr A diffuse complex with no clear soft X-ray counterparts. The severe extinction observed in the Chandra spectra indicates that all the NuSTAR sources are in the central bulge or are of extragalactic origin. Spectral analysis of relatively bright NuSTAR sources suggests that magnetic cataclysmic variables constitute a large fraction (>40%–60%). Both spectral analysis and logN–logS distributions of the NuSTAR sources indicate that the X-ray spectra of the NuSTAR sources should have kT > 20 keV on average for a single temperature thermal plasma model or an average photon index of Γ = 1.5–2 for a power-law model. These findings suggest that the GC X-ray source population may contain a larger fraction of XBs with high plasma temperatures than the field population.
OSTI ID:
22868907
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 825; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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Cited By (13)

Galactic binaries can explain the Fermi Galactic centre excess and 511 keV emission journal August 2018
The Galactic Bulge Diffuse Emission in Broad-Band X-rays with NuSTAR text January 2019
The NuSTAR Serendipitous Survey: The 40-month Catalog and the Properties of the Distant High-energy X-Ray Source Population journal February 2017
Observatory science with eXTP text January 2018
NuSTAR and Chandra Observations of New X-Ray Transients in the Central Parsec of the Galaxy journal November 2019
X-ray detectability of accreting isolated black holes in our Galaxy journal March 2018
Evidence for Intermediate Polars as the Origin of the Galactic Center hard X-Ray Emission journal July 2016
Almost closing the ν MSM sterile neutrino dark matter window with NuSTAR journal June 2017
Searching for Primordial Black Holes in the radio and X-ray sky text January 2016
A density cusp of quiescent X-ray binaries in the central parsec of the Galaxy journal April 2018
Neutron Stars and Black Holes in the Small Magellanic Cloud: The SMC NuSTAR Legacy Survey journal October 2019
Investigating the origin of the faint non-thermal emission of the Arches cluster using the 2015-2016 NuSTAR and XMM-Newton X-ray observations text January 2019
Spitzer Infrared Spectrograph Observations of the Galactic Center: Quantifying the Extreme Ultraviolet/so ft X-ray fluxes text January 2018


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