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Proposal ID 080101
Title The onset of magnetic activity in X-rays - From late A to early F stars
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DOI https://doi.org/10.5270/esa-0wm30ic
Principal Investigator, PI Dr Jan Robrade
Abstract We propose to observe a sample of late A to early F stars with XMM-Newton tosystematically investigate coronal properties at the onset of stellar magneticactivity in X-rays. These stars feature a thin or localized outer convectionzone and have been only poorly explored by modern X-ray instruments. We focus onnearby, presumably single main-sequence stars with well known stellarparameters. The aim is to study the interplay between developing convectiveenvelope and rotation, thereby driving a stellar dynamo mechanism and generatingcoronal X-ray emission.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2017-08-23T15:43:20Z/2017-12-18T08:06:57Z
Version 21.51_20241115_1113
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 2019-01-15T23:00:00Z
Last Update 2026-07-09
Keywords "thereby driving", "coronal properties", "XMM-Newton", "stellar magnetic activity", "stellar parameters", "poorly explored", "magnetic activity", "XMM", "stellar dynamo mechanism", "modern xray instruments", "developing convective envelope", "xmm newton"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Jan Robrade, 2019, 'The onset of magnetic activity in X-rays - From late A to early F stars', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-0wm30ic
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.