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Related papers: Nucleosynthesis in Type I X-ray Bursts

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The past decade and a half has seen many interesting new developments in X-ray burst research, both observationally and theoretically. New phenomena were discovered, such as burst oscillations and superbursts, and new regimes of…

High Energy Astrophysical Phenomena · Physics 2011-02-17 Jean in 't Zand

This overview discusses issues relevant to modeling nucleosynthesis in type II supernovae and implications of detailed studies of the ejecta. After a brief presentation of the most common approaches to stellar evolution and parameterized…

Astrophysics · Physics 2007-05-23 T. Rauscher

Because calibrated light curves of Type Ia supernovae have become a major tool to determine the local expansion rate of the Universe and also its geometrical structure, considerable attention has been given to models of these events over…

Astrophysics · Physics 2008-11-26 W. Hillebrandt , J. C. Niemeyer

Runaway thermonuclear burning of a layer of accumulated fuel on the surface of a compact star provides a brief but intense display of stellar nuclear processes. For neutron stars accreting from a binary companion, these events manifest as…

Recent studies have shown that runaway thermonuclear burning of material accreted onto neutron stars, i.e. Type I X-ray bursts, may affect the accretion disk. We investigate this by performing a detailed time-resolved spectral analysis of…

High Energy Astrophysical Phenomena · Physics 2015-06-19 L. Keek , D. R. Ballantyne , E. Kuulkers , T. E. Strohmayer

Oscillations in the X-ray flux of thermonuclear X-ray bursts have been observed with RXTE from at least 6 low-mass binaries, at frequencies from 330 Hz to 589 Hz. There appear to be preferred relations between the frequencies present during…

Astrophysics · Physics 2009-10-30 T. E. Strohmayer , J. H. Swank , W. Zhang

A small subset of thermonuclear X-ray bursts on neutron stars exhibit such a strong photospheric expansion that for a few seconds the photosphere is located at a radius r_ph >~ 1000 km. Such `superexpansions' imply a large and rapid energy…

High Energy Astrophysical Phenomena · Physics 2015-05-14 J. J. M. in 't Zand , N. N. Weinberg

Type Ia supernovae are associated with thermonuclear explosions of white dwarf stars. Combustion processes convert material in nuclear reactions and release the energy required to explode the stars. At the same time, they produce the…

Solar and Stellar Astrophysics · Physics 2018-04-25 Friedrich K. Roepke

The millisecond pulsar MAXI J1816-195 was recently discovered in an outburst by MAXI in 2022 May. We study different properties of the pulsar using data from NuSTAR and NICER observations. The unstable burning of accreted material on the…

High Energy Astrophysical Phenomena · Physics 2023-02-28 Manoj Mandal , Sabyasachi Pal , Jaiverdhan Chauhan , Anne Lohfink , Priya Bharali

We investigate the latitude at which type I X-ray bursts are ignited on rapidly rotating accreting neutron stars. We find that, for a wide range of accretion rates, ignition occurs preferentially at the equator, in accord with the work of…

Astrophysics · Physics 2009-11-13 Randall L. Cooper , Ramesh Narayan

Relativistic jets are observed from accreting and cataclysmic transients throughout the Universe, and have a profound affect on their surroundings. Despite their importance, their launch mechanism is not known. For accreting neutron stars,…

Type I X-ray bursts are produced by thermonuclear runaways that develop on accreting neutron stars. Once one location ignites, the flame propagates across the surface of the star. Flame propagation is fundamental in order to understand…

High Energy Astrophysical Phenomena · Physics 2016-05-02 Yuri Cavecchi , Yuri Levin , Anna L. Watts , Jonathan Braithwaite

Nuclear reactions in accreting neutron-star crusts and the heat release accompanying them are studied, under different assumptions concerning the composition of the outermost layer formed of the ashes of X-ray bursts. Particular examples of…

Astrophysics · Physics 2011-05-23 P. Haensel , J. L. Zdunik

Now 50 years since the existence of the neutron star crust was proposed, we review the current understanding of the nuclear physics of the outer layers of accreting neutron stars. Nuclei produced during nuclear burning replace the nascent…

High Energy Astrophysical Phenomena · Physics 2018-08-09 Zach Meisel , Alex Deibel , Laurens Keek , Peter Shternin , Justin Elfritz

Type-I X-ray bursts can be used to determine properties of accreting neutron stars via comparisons between model calculations and astronomical observations, exploiting the sensitivity of models to astrophysical conditions. However, the…

High Energy Astrophysical Phenomena · Physics 2019-02-19 Zach Meisel , Grant Merz , Sophia Medvid

The pattern of nucleosynthesis during the explosion of a low-mass neutron star formed in a close binary system in the stripping scenario is considered. In the scenario considered the shock arising during the explosion is shown to strongly…

High Energy Astrophysical Phenomena · Physics 2024-11-05 Igor Panov , Anton Ignatovskiy , Andrey Yudin

We investigate the thermonuclear bursting behaviour of IGR J17473-2721, an X-ray transient that in 2008 underwent a six month long outburst, starting (unusually) with an X-ray burst. We detected a total of 57 thermonuclear bursts throughout…

High Energy Astrophysical Phenomena · Physics 2010-12-24 J. Chenevez , D. Altamirano , D. K. Galloway , J. J. M. in 't Zand , E. Kuulkers , N. Degenaar , M. Falanga , E. Del Monte , Y. Evangelista , M. Feroci , E. Costa

Precision measurements of neutron star radii can provide a powerful probe of the properties of cold matter beyond nuclear density. Beginning in the late 1970s it was proposed that the radius could be obtained from the apparent or inferred…

High Energy Astrophysical Phenomena · Physics 2015-05-14 Sudip Bhattacharyya , M. Coleman Miller , Duncan K. Galloway

Swift J1749.4-2807 is the only known eclipsing accreting millisecond X-ray pulsar. In this paper, we report on 7 thermonuclear (Type-I) X-ray bursts observed by NICER during its 2021 outburst. The first 6 bursts show slow rises and long…

High Energy Astrophysical Phenomena · Physics 2023-06-28 A. C. Albayati , P. Bult , D. Altamirano , J. Chenevez , S. Guillot , T. Güver , G. K. Jaisawal , C. Malacaria , G. C. Mancuso , A. Marino , M. Ng , A. Sanna , T. E. Strohmayer

The neutron star X-ray binary, EXO 0748--676, was observed regularly by the Rossi X-ray Timing Explorer (RXTE) and XMM-Newton during its first detected outburst (1985 - 2008). These observations captured hundreds of asymmetric,…

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