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Proposal ID 086504
Title T-Rex\\: Time-resolved Radiation Environment of planet forming disks with XMM
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DOI https://doi.org/10.57780/esa-s3gcs8h
Principal Investigator, PI Dr Christian Schneider
Abstract X-ray emission from young stars is a crucial agent in the formation of planetarysystems, driving the chemistry and eventual dispersal of protoplanetary disks.K2.s 80-day monitoring of young stars in the Taurus star-forming region showsdramatic variability that points to changes in levels of accretion,circumstellar absorption and magnetic activity on timescales of days to weeks.Similar variability is expected in X-rays, causing important changes in thehigh-energy irradiation of planet-forming disks, but is largely unexplored inX-rays. Therefore, we propose the first large-scale X-ray monitoring campaign ofwell-characterized T Tauri stars with this cadence.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2020-08-18T13:32:46Z/2020-09-19T02:20:12Z
Version 18.02_20200221_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 2021-10-27T00:00:00Z
Keywords "energy irradiation", "XMM", "circumstellar absorption", "planetary systems", "scale xray", "planet forming dis", "tauri stars", "xray emission", "magnetic activity", "protoplanetary dis", "eventual dispersal"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Christian Schneider, 2021, 'T-Rex\\: Time-resolved Radiation Environment of planet forming disks with XMM', 18.02_20200221_1200, European Space Agency, https://doi.org/10.57780/esa-s3gcs8h