Type I X-ray Bursts Detected by the JEM-X Telescope Onboard the INTEGRAL Observatory in 2003–2015
| Autor: | I. V. Chelovekov, A. V. Prosvetov, S. A. Grebenev, Ilya A. Mereminskiy |
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| Rok vydání: | 2017 |
| Předmět: |
Physics
education.field_of_study 010308 nuclear & particles physics Astrophysics::High Energy Astrophysical Phenomena Population X-ray Astronomy and Astrophysics Astrophysics Light curve 01 natural sciences Luminosity law.invention Telescope Accretion rate Neutron star Space and Planetary Science Observatory law 0103 physical sciences education 010303 astronomy & astrophysics |
| Zdroj: | Astronomy Letters. 43:781-795 |
| ISSN: | 1562-6873 1063-7737 |
| DOI: | 10.1134/s1063773717120076 |
| Popis: | We present the results of our analysis of the JEM-X/INTEGRAL data obtained from January 2003 to January 2015 aimed at searching for type I X-ray bursts from known and new bursters. Such bursts are caused by thermonuclear explosions on the surface of a neutron star. We have searched for bursts in the records of the count rate of the JEM-X detectors in the 3–20 keV energy band. We have separately reconstructed and analyzed the light curves of 104 X-ray bursters known to date based on the JEM-X data. A similar search for bursts was previously carried out in the 15–25 keV data from the IBIS/ISGRI telescope onboard the INTEGRAL observatory obtained in 2003–2009. We have continued to analyze the data from this telescope up until the observations in January 2015. The joint catalog of bursts detected by the two instruments includes 2201 events; their basic parameters are given. The large size of the sample of bursts makes it one of the most representative of the existing one and allows various statistical studies of bursts to be performed. In particular, we have constructed the dependence of the mean rate of type I bursts from bursters on the luminosity (accretion rate), revealed an appreciable burst rate from sources with a near-Eddington luminosity, and investigated the population of multiple bursts with a recurrence time much shorter than the time it takes for a critical mass of matter required for the initiation of an explosion to be accumulated on the neutron star surface. Almost all of the detected bursts are associated with already known bursters,we have found only one previously unknown burster, IGRJ17380-3749, in the archival data, and one more known, but poorly studied source, AX J1754.2-2754, has been identified as a burster. Several similar sources have previously been identified as bursters directly during the INTEGRAL observations. |
| Databáze: | OpenAIRE |
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