A deficit of type I X-ray bursts from low-accretion-rate binaries: Data from the TTM/COMIS telescope onboard the Mir-Kvant observatory |
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| Authors: | A N Emelyanov V A Aref’ev E M Churazov M R Gilfanov R A Sunyaev |
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| Institution: | (1) Space Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow, 117810, Russia;(2) Max-Planck-Institut für Astrophysik, Karl Schwarzschild Strasse 1, 86740 Garching bei München, Germany |
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| Abstract: | We analyze 175 sessions of Galactic-center observations with the TTM/COMIS telescope onboard the Mir-Kvant observatory from 1987 until 1998. Because of its wide field of view (～ 15°×15°), much of the Galaxy and, hence, a large number of X-ray sources were simultaneously within the telescope aperture. During the observations, 47 X-ray bursts were detected, 33 of which are most likely type I bursts related to unstable helium burning on the surfaces of neutron stars. All the detected type I bursts were identified with known X-ray sources; the pre-and post-burst luminosities of these sources measured with the TTM telescope were high. No bursts were detected from voids, i.e., from sources whose luminosities in quiescence did not exceed the TTM detection threshold. This result allows us to constrain the combination of the number of binary sources with low accretion rates and the properties of X-ray bursts from such sources, in particular, the peak luminosity during bursts and the frequency of their occurrence. |
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| Keywords: | Mir-Kvant Roentgen TTM neutron stars X-ray binaries bursters accretion type I bursts |
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