A dataset provided by the European Space Agency

Name 088380
Title Testing the steep decline in chromospheric emission of very late M dwarfs
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883800101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883800201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883800301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883800401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883800501

DOI https://doi.org/10.57780/esa-esnyv3o
Author Prof Peter Wheatley
Description We recently published evidence for a steep decline in chromospheric ultraviolet
emission compared with coronal X-ray emission for mid-to-late M dwarfs. Very
late M dwarfs appear to be underluminous in the ultraviolet by two orders of
magnitude. If confirmed, this chromospheric decline will have profound
implications for the habitability of exoplanet systems similar to TRAPPIST-1.
The chromospheric decline may also point to a change in stellar dynamo mechanism
at the fully convective boundary. We propose XMM-Newton and HST observations of
three very late M dwarfs in order to test that the chromospheric decline is a
common feature of the class.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-06-24T14:34:06Z/2022-02-22T18:30:21Z
Version 19.17_20220121_1250
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 2023-03-22T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Peter Wheatley, 2023, 088380, 19.17_20220121_1250, European Space Agency, https://doi.org/10.57780/esa-esnyv3o