A dataset provided by the European Space Agency

Name 001145
Title Reprocessed X-Rays from the Disk and Highly Disrupted Wind of SMC X-1/Sk 160
URL

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
Author European Space Agency
Description The circumstellar environment of SMC X-1 contains both a highly disrupted
stellar wind and an accretion disk putting it in a class containing only three
X-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 excellent
spectral sensitivity of XMM down to 350 eV make for an especially powerful probe
of this material down to low ionization levels through spectral features from
K shell transitions in carbon, nitrogen, and oxygen. We propose one 50 ksec
observation of SMC X-1 over an eclipse to study the extended wind and one 30
ksec observation outside of eclipse to study material near the neutron star.
Publication No observations found associated with the current proposal
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 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 2003-02-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 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