A dataset provided by the European Space Agency

Name 080027
Title A Comprehensive Survey of Accretion in Double White Dwarfs
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800270501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800270601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800270701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800270801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800271001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800271101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800271401

DOI https://doi.org/10.5270/esa-21sb8uf
Author Prof Thomas Maccarone
Description At the present time, the X-ray measurements of AM CVn stars (systems where one
white dwarf accretes from another white dwarf) are heavily biased toward short
period systems. We propose to recitfy the situation by observing all AM CVn
stars which do not have XMM observations in the archives but do have known
periods. In fact, the X-ray measurements are more important for the long period
systems than the short period systems, since in the long period systems, the
boundary layers are expected to be optically thin, and a much larger fraction of
the bolometric luminosity is expected to come out in X-rays, meaning that using
these systems to test our understanding of evolution of double white dwarfs
depends crucially on knowing their X-ray fluxes.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2017-09-06T17:21:56Z/2018-04-16T17:47:59Z
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 2019-05-09T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Thomas Maccarone, 2019, 080027, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-21sb8uf