A dataset provided by the European Space Agency

Name: Reprocessed X-Rays from the Disk and Highly Disrupted Wind of SMC X-1/Sk 160
Published: 2003-02-02T00:00:00Z

Proposal ID	001145
Title	Reprocessed X-Rays from the Disk and Highly Disrupted Wind of SMC X-1/Sk 160
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0011450101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0011450201
DOI	https://doi.org/10.5270/esa-pcsosi0
Principal Investigator, PI	Dr Patrick Wojdowski
Abstract	The circumstellar environment of SMC X-1 contains both a highly disruptedstellar wind and an accretion disk putting it in a class containing only threeX-ray pulsars. X-ray reprocessing in this material provide a probe of this material. The small absorbing column density to SMC X-1 and the excellentspectral sensitivity of XMM down to 350 eV make for an especially powerful probeof this material down to low ionization levels through spectral features fromK shell transitions in carbon, nitrogen, and oxygen. We propose one 50 ksecobservation of SMC X-1 over an eclipse to study the extended wind and one 30ksec observation outside of eclipse to study material near the neutron star.
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Q. et al. \| ApJ \| 961-130 \| 2024 \| 2024ApJ...961..130Z \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..130Z The MeerKAT 1.3 GHz Survey of the Small Magellanic Cloud \|Cotton W. D. Filipoviu0107 M. 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Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2001-05-31T02:13:48Z/2001-11-16T14:50:44Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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	2003-02-02T00:00:00Z
Last Update	2025-01-27
Keywords	"disrupted wind", "disrupted stellar wind", "low ionization levels", "especially powerful probe", "spectral sensitivity", "sk 160", "accretion disk putting", "absorbing column density", "smc x", "shell transitions", "reprocessed xray", "xray reprocessing", "XMM", "xray pulsars", "neutron star"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Patrick Wojdowski, 2003, 'Reprocessed X-Rays from the Disk and Highly Disrupted Wind of SMC X-1/Sk 160', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-pcsosi0