A dataset provided by the European Space Agency

Name 078051
Title Dependence of Coronal Element Fractionation on Metallcity
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780510101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780510301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780510401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0780510501

DOI https://doi.org/10.5270/esa-c99zjdk
Author Prof Ehud Behar
Description We propose to study elemental fractionation between the photosphere and the corona in stars with super-solar abundances, and their dependence on the First Ionization Potential (FIP). Currently, coronal abundances have been measured for only 3 stars with average metallicity of [A Z -A H ] > 0.3. We propose to observe 5 additional metal rich stars in order to understand whether high atmospheric abundances affect coronal composition. The immediate goal of the proposed observations is to determine the coronal enrichment and depletion factor(s) for confirmed high-metallicity stars, compare them with those previously found for stars with solar abundances and measure (or exclude) the dependence of the process(es) causing coronal fractionation on metallicity.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2016-09-30T15:38:09Z/2017-03-16T11:43:14Z
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 2018-04-12T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2018-04-12T22:00:00Z, 078051, 17.56_20190403_1200. https://doi.org/10.5270/esa-c99zjdk