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Related papers: Models for Type I X-Ray Bursts with Improved Nucle…

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A type-I burst could influence the accretion process through radiation pressure and Comptonization both for the accretion disk and the corona/boundary layer of an X-ray binary, and vice versa. We investigate the temporal evolution of a…

High Energy Astrophysical Phenomena · Physics 2022-09-07 Yu-Peng Chen , Shu Zhang , Long Ji , Shuang-Nan Zhang , Ling-Da Kong , Peng-Ju Wang , Zhi Chang , Jing-Qiang Peng , Jian Li , Jin-Lu Qu

We report an analysis of Insight-HXMT observations of the newly discovered accreting millisecond pulsar SRGA J144459.2$-$604207. During the outburst, detected in 2024 February by SRG/ART-XC, the broadband persistent spectrum was well fitted…

We present multidimensional simulations of the early convective phase preceding ignition in a Type I X-ray burst using the low Mach number hydrodynamics code, MAESTRO. A low Mach number approach is necessary in order to perform long-time…

High Energy Astrophysical Phenomena · Physics 2015-05-20 C. M. Malone , A. Nonaka , A. S. Almgren , J. B. Bell , M. Zingale

The strong degeneracy of the 12C ignition layer on an accreting neutron star results in a hydrodynamic thermonuclear runaway, in which the nuclear heating time becomes shorter than the local dynamical time. We model the resulting combustion…

Astrophysics · Physics 2009-11-13 Nevin N. Weinberg , Lars Bildsten

We study 15 thermonuclear X-ray bursts from 4U 1820--30 observed with the Neutron Star Interior Composition Explorer (NICER). We find evidence of a narrow emission line at 1.0 keV and three absorption lines at 1.7, 3.0, and 3.75 keV,…

We use new central stellar velocity dispersions and nuclear X-ray and Halpha luminosities for the Palomar survey of nearby galaxies to investigate the distribution of nuclear bolometric luminosities and Eddington ratios for their central…

Astrophysics of Galaxies · Physics 2009-07-17 Luis C. Ho

We perform a set of numerical experiments studying the interaction of Type I X-ray bursts with thin, Shakura-Sunyaev type accretion discs. Careful observations of X-ray spectra during such bursts have hinted at changes occurring in the…

High Energy Astrophysical Phenomena · Physics 2020-01-07 P. Chris Fragile , David R. Ballantyne , Aidan Blankenship

We analyzed 123 thermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer from the low-mass X-ray binary 4U 1636-536. All but two of the 40 radius-exansion bursts in this sample reached peak fluxes which were normally…

Astrophysics · Physics 2009-11-13 Duncan Galloway , Dimitrios Psaltis , Michael P. Muno , Deepto Chakrabarty

Neutron stars in close binary star systems often accrete matter from their companion stars. Thermonuclear ignition of the accreted material in the atmosphere of the neutron star leads to a thermonuclear explosion which is observed as an…

Since the discovery of the accreting millisecond pulsar XTE J1814-338 a total of 27 thermonuclear bursts have been observed from the source with the Proportional Counter Array (PCA) onboard the Rossi X-ray Timing Explorer (RXTE).…

Astrophysics · Physics 2009-11-10 Tod E. Strohmayer , Craig B. Markwardt , Jean H. Swank , Jean in 't Zand

Two flares with a duration of several hours are reported for the low-mass X-ray binary 4U 1636-53. The characteristics of these flares (i.e., decay time scales, spectral softening, fluences) are very similar to the very long type-I X-ray…

Astrophysics · Physics 2009-11-06 Rudy Wijnands

MAXI J1807+132 is a low-mass X-ray binary (LMXB) first detected in outburst in 2017. Observations during the 2017 outburst did not allow for an unambiguous identification of the nature of the compact object. MAXI J1807+132 was detected in…

We present estimates for the accretion rates in 13 X--ray bursting sources which exhibit photospheric expansion, basing on theoretical models of stationary, radiatively driven winds from neutron stars. The relatively high values obtained,…

Astrophysics · Physics 2009-10-22 Iosif Lapidus , Luciano Nobili , Roberto Turolla

We examine unresolved nuclear X-ray sources in 57 brightest cluster galaxies to study the relationship between nuclear X-ray emission and accretion onto supermassive black holes (SMBHs). The majority of the clusters in our sample have…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 H. R. Russell , B. R. McNamara , A. C. Edge , M. T. Hogan , R. A. Main , A. N. Vantyghem

When neutron stars (NS) accrete gas from low-mass binary companions, explosive nuclear burning reactions in the NS envelope fuse hydrogen and helium into heavier elements. The resulting thermonuclear (type-I) X-ray bursts produce energy…

High Energy Astrophysical Phenomena · Physics 2016-10-05 J. J. E. Kajava , J. Nättilä , J. Poutanen , A. Cumming , V. Suleimanov , E. Kuulkers

Hotspots on the surface of accreting neutron stars have been directly observed via pulsations in the lightcurves of X-ray pulsars. They are thought to occur due to magnetic channelling of the accreted fuel to the neutron star magnetic…

High Energy Astrophysical Phenomena · Physics 2021-07-14 A. J. Goodwin , A. Heger , F. R. N. Chambers , A. L. Watts , Y. Cavecchi

We study a sample of 44 low-luminosity radio-loud AGN, which represent a range of nuclear radio-power spanning 5 orders of magnitude, to unveil the accretion mechanism in these galaxies. We estimate the accretion rate of gas associated with…

Astrophysics · Physics 2009-11-13 Barbara Balmaverde , Ranieri D. Baldi , Alessandro Capetti

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

Nucleosynthesis in Type I X-ray bursts may involve up to several thousand nuclear processes. The majority of these processes have only been determined theoretically due to the lack of sufficient experimental information. Accurate reaction…

Astrophysics · Physics 2009-11-13 A. Parikh , J. Jose , C. Iliadis , F. Moreno , T. Rauscher

We present a study of weak, thermonuclear X-ray bursts from the accreting millisecond X-ray pulsar SAX J1808.4-3658. We focus on a burst observed with the Neutron Star Interior Composition Explorer on 2019 August 9, and describe a similar…

High Energy Astrophysical Phenomena · Physics 2023-05-26 Sierra Casten , Tod Strohmayer , Peter Bult