A dataset provided by the European Space Agency

Name 072283
Title First View of the Accretion Disks in Normal Symbiotic Stars
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722830101

DOI https://doi.org/10.5270/esa-6c7o617
Author European Space Agency
Description Accretion disks in symbiotic stars are often hidden by the bright optical
emission from the red-giant companion, UV emission from the ionized nebula, and
soft (E < 2 keV) X-rays from colliding winds. A survey with Swift, however, has
revealed that the accretion disks dominates above 2 keV, as well as in the
rapidly variable portion of the UV light. Our proposed simultaneous X-ray and UV
observations of 3 targets from the Swift survey with XMM-Newton is uniquely
suited to pioneer the study of these important disks and determine the range of
accretion rates in symbiotics; compare the properties of the flickering with
other disk accretors; and confirm the primary results of the Swift survey. This
research has implications for the physics of accretion disks and symbiotics as SNIa progenitors.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-12-01T10:08:03Z/2013-12-02T03:09:43Z
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 2014-12-20T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014, First View Of The Accretion Disks In Normal Symbiotic Stars, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6c7o617