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Article Dans Une Revue Proceedings of the International Astronomical Union Année : 2013

The 3 Ms Chandra campaign on Sgr A*: a census of X-ray flaring activity from the Galactic center

J. Neilsen,
  • Fonction : Auteur
C. Gammie,
  • Fonction : Auteur
J. Dexter,
  • Fonction : Auteur
S. Markoff,
  • Fonction : Auteur
D. Haggard,
  • Fonction : Auteur
S. Nayakshin,
  • Fonction : Auteur
D. Wang, Q.
  • Fonction : Auteur
N. Grosso,
A. Tomsick, J.
  • Fonction : Auteur
N. Degenaar,
  • Fonction : Auteur
C. Fragile, P.
  • Fonction : Auteur
C. Houck, J.
  • Fonction : Auteur
R. Wijnands,
  • Fonction : Auteur
M. Miller, J.
  • Fonction : Auteur
K. Baganoff, F.
  • Fonction : Auteur

Résumé

Over the last decade, X-ray observations of Sgr A* have revealed a black hole in a deep sleep, punctuated roughly once per day by brief flares. The extreme X-ray faintness of this supermassive black hole has been a long-standing puzzle in black hole accretion. To study the accretion processes in the Galactic center, Chandra (in concert with numerous ground- and space-based observatories) undertook a 3 Ms campaign on Sgr A* in 2012. With its excellent observing cadence, sensitivity, and spectral resolution, this Chandra X-ray Visionary Project (XVP) provides an unprecedented opportunity to study the behavior of the closest supermassive black hole. We present a progress report from our ongoing study of X-ray flares, including the brightest flare ever seen from Sgr A*. Focusing on the statistics of the flares and the quiescent emission, we discuss the physical implications of X-ray variability in the Galactic center.

Dates et versions

hal-02327542 , version 1 (22-10-2019)

Identifiants

Citer

J. Neilsen,, A. Nowak, M., C. Gammie,, J. Dexter,, S. Markoff,, et al.. The 3 Ms Chandra campaign on Sgr A*: a census of X-ray flaring activity from the Galactic center. Proceedings of the International Astronomical Union, 2013, 9 (S303), pp.374-378. ⟨10.1017/S1743921314000945⟩. ⟨hal-02327542⟩
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