A catalogue of unusually long thermonuclear bursts on neutron stars

Author:

Alizai K1ORCID,Chenevez J1,Cumming A2,Degenaar N3,Falanga M4ORCID,Galloway D K5,in ’t Zand J J M6,Jaisawal G K1ORCID,Keek L7,Kuulkers E8,Lampe N5,Schatz H9,Serino M10

Affiliation:

1. National Space Institute, Technical University of Denmark , Elektrovej 327, 2800 Kongens Lyngby, Denmark

2. Physics Dept., McGill University , 3600 Rue University, Montreal, QC, H3A 2T8, Canada

3. Anton Pannekoek Institute for Astronomy, University of Amsterdam , Postbus 94249, NL-1090 GE Amsterdam, the Netherlands

4. International Space Science Institute , Hallerstrasse 6, 3012 Bern, Switzerland

5. School of Physics & Astronomy, Monash University , VIC 3800, Australia

6. SRON Netherlands Institute for Space Research , Niels Bohrweg 4, 2333 CA Leiden, The Netherlands

7. Cosine measurement systems , Oosteinde 36, Warmond, 2361 HE, The Netherlands

8. ESA/ESTEC , Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands

9. Dept. of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University , East Lansing, MI 48824

10. Department of Physics and Mathematics, Aoyama Gakuin University , 5-10-1 Fuchinobe, Chuo-ku, Sagamihara, Kanagawa 252-5258, Japan

Abstract

ABSTRACT 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 (≈1010 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 1040 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.

Funder

NASA

NWO

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. Dark matter in compact stars;Physics Reports;2024-02

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