A dataset provided by the European Space Agency

Name: Dependence of Coronal Element Fractionation on Metallcity
Published: 2018-04-12T22:00:00Z

Proposal ID	078051
Title	Dependence of Coronal Element Fractionation on Metallcity
Download Data Associated to the proposal	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
Principal Investigator, PI	Prof Ehud Behar
Abstract	We propose to study elemental fractionation between the photosphere and thecorona in stars with super-solar abundances, and their dependence on the FirstIonization Potential (FIP). Currently, coronal abundances have been measured foronly 3 stars with average metallicity of A Z /A H > 0.3. We propose toobserve 5 additional metal rich stars in order to understand whether highatmospheric abundances affect coronal composition. The immediate goal of theproposed observations is to determine the coronal enrichment and depletionfactor(s) for confirmed high-metallicity stars, compare them with thosepreviously found for stars with solar abundances and measure (or exclude) thedependence of the process(es) causing coronal fractionation on metallicity.
Publications	Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Tidal star-planet interaction and its observed impact on stellar activity in planet-hosting wide binary systems \|Ilic, N., Poppenhaeger, K., \| MNRAS \| 513-4380 \| 2022 \| 2022MNRAS.513.4380I \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.4380I The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 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	2018-04-12T22:00:00Z
Keywords	"average metallicity", "elemental fractionation", "coronal element fractionation", "coronal abundance", "solar abundance", "ionization potential fip", "depletion factors", "super solar abundance", "coronal enrichment"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Ehud Behar, 2018, 'Dependence of Coronal Element Fractionation on Metallcity', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-c99zjdk