A catalogue of unusually long thermonuclear bursts on neutron stars

被引:11
作者
Alizai, K. [1 ]
Chenevez, J. [1 ]
Cumming, A. [2 ]
Degenaar, N. [3 ]
Falanga, M. [4 ]
Galloway, D. K. [5 ]
in 't Zand, J. J. M. [6 ]
Jaisawal, G. K. [1 ]
Keek, L. [7 ]
Kuulkers, E. [8 ]
Lampe, N.
Schatz, H. [9 ,10 ]
Serino, M. [11 ]
机构
[1] Tech Univ Denmark, Natl Space Inst, Elektrovej 327, DK-2800 Lyngby, Denmark
[2] McGill Univ, Phys Dept, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada
[3] Univ Amsterdam, Anton Pannekoek Inst Astron, Postbus 9424, NL-1090 GE Amsterdam, Netherlands
[4] Int Space Sci Inst, Hallerstr 6, CH-3012 Bern, Switzerland
[5] Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
[6] SRON Netherlands Inst Space Res, Niels Bohrweg 4, NL-2333 CA Leiden, Netherlands
[7] Cosine measurement Syst, Oosteinde 36, NL-2361 HE Warmond, Netherlands
[8] ESA ESTEC, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands
[9] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[10] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA
[11] Aoyama Gakuin Univ, Dept Phys & Math, 5-10-1 Fuchinobe,Chuo Ku, Sagamihara, Kanagawa 2525258, Japan
关键词
X-ray: binaries; X-ray: bursts; stars: neutron; X-RAY-BURSTS; NEAR-INFRARED COUNTERPART; ORBITAL PERIOD; CHANDRA OBSERVATIONS; ABSORPTION FEATURES; PERSISTENT EMISSION; MILLISECOND PULSAR; SPECTRAL EVOLUTION; GLOBULAR-CLUSTERS; GALACTIC BULGE;
D O I
10.1093/mnras/stad374
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Rare, energetic (long) thermonuclear (Type I) X-ray bursts are classified either as intermediate-duration or 'supern' bursts, based on their duration. Intermediate-duration bursts lasting a few to tens of minutes are thought to arise from the thermonuclear runaway of a relatively thick (approximate to 10(10) g cm(-2)) helium layer, while superbursts lasting hours are attributed to the detonation of an underlying carbon layer. We present a catalogue of 84 long thermonuclear bursts from 40 low-mass X-ray binaries, and defined from a new set of criteria distinguishing them from the more frequent short bursts. The three criteria are: (1) a total energy release longer than 10(40) erg, (2) a photospheric radius expansion phase longer than 10 s, and (3) a burst time-scale longer than 70 s. This work is based on a comprehensive systematic analysis of 70 bursts found with INTEGRAL, RXTE, Swift, BeppoSAX, MAXI, and NICER, as well as 14 long bursts from the literature that were detected with earlier generations of X-ray instruments. For each burst, we measure its peak flux and fluence, which eventually allows us to confirm the distinction between intermediate-duration bursts and superbursts. Additionally, we list 18 bursts that only partially meet the above inclusion criteria, possibly bridging the gap between normal and intermediate-duration bursts. With this catalogue, we significantly increase the number of long-duration bursts included in the MINBAR and thereby provide a substantial sample of these rare X-ray bursts for further study.
引用
收藏
页码:3608 / 3624
页数:17
相关论文
共 220 条
[1]   A catalogue of intermediate-duration Type I X-ray bursts observed with the INTEGRAL satellite [J].
Alizai, K. ;
Chenevez, J. ;
Brandt, S. ;
Lund, N. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 494 (02) :2509-2522
[2]   A superburst candidate in EXO 1745-248 as a challenge to thermonuclear ignition models [J].
Altamirano, D. ;
Keek, L. ;
Cumming, A. ;
Sivakoff, G. R. ;
Heinke, C. O. ;
Wijnands, R. ;
Degenaar, N. ;
Homan, J. ;
Pooley, D. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 426 (02) :927-934
[3]   Time-resolved ultraviolet observations of the globular cluster x-ray source in NGC 6624: The shortest known period binary system [J].
Anderson, SF ;
Margon, B ;
Deutsch, EW ;
Downes, RA ;
Allen, RG .
ASTROPHYSICAL JOURNAL, 1997, 482 (01) :L69-L72
[4]  
[Anonymous], 1995, X-ray Binaries
[5]  
[Anonymous], 2008, POS INTEGRAL08
[6]  
ArmasPadilla M., 2013, MNRAS, V434, P1586, DOI [10.1093/mnras/stt1114, DOI 10.1093/MNRAS/STT1114]
[7]  
Arnaud KA, 1996, ASTR SOC P, V101, P17
[8]  
Asada M., 2011, ASTRON TELEGRAM, V3760
[9]   Iron K emission lines in the energy spectra of low-mass X-ray binaries observed with ASCA [J].
Asai, K ;
Dotani, T ;
Nagase, F ;
Mitsuda, K .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2000, 131 (02) :571-591
[10]  
Augusteijn T, 1998, ASTRON ASTROPHYS, V332, P561