A dataset provided by the European Space Agency

Name 070119
Title Helium-rich thermonuclear bursts from the Slow Burster
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701190101

DOI 10.5270/esa-stqsuwb
Author Dr Duncan Galloway
Description Thermonuclear bursts in systems accreting pure helium reveal the structure of the neutron star (NS) interiors. Without heating from steady H-burning between bursts, the burst recurrence times and energetics are more sensitive to the thermal properties and processes in the NS crust and core. Burst ignition models predict longer burst recurrence times than observed which may be due to fractional covering of the accreted fuel on the NS surface, supported by recent analyses of several bursts from 4U 172834. But other processes including steady He-burning or incomplete burning, may also be important. Simultaneous INTEGRAL-XMM observations of 4U 172834 allow measurements of the burst recurrence time and accretion rate, to distinguish between these possibilities.
Publication The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
A Study of Low-mass X-Ray Binaries in the Low-luminosity Regime . Sonbas, E., Dhuga, K. S., . ApJ . 853-150 . 2018 . 2018ApJ...853..150S ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-10-02T01:25:12Z/2013-10-02T05:01:52Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2014-10-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-10-17T00:00:00Z, 070119, 17.56_20190403_1200. https://doi.org/10.5270/esa-stqsuwb