A dataset provided by the European Space Agency

Name 088170
Title Fraternal or Identical? The Magnetic Properties of M Dwarf Twins
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881700101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881700201

DOI https://doi.org/10.57780/esa-awtxc3g
Author European Space Agency
Description We propose for 68 ksec of observing time on XMM-Newton to monitor X-ray activity
on four pairs of virtually identical twin M dwarfs. These twin wide binaries are
comprised of stars with nearly identical masses, ages, and compositions.
Evolutionary models and conventional thinking suggest that such sets of twin
stars should evolve nearly co-equally, resulting in similar levels of magnetic
activity. These XMM-Newton data will be used in concert with optical monitoring
that provides information about short-term flaring, medium-term rotation
periods, and long-term stellar spot cycles, which can then be correlated with
X-ray activity. This work is carried out as part of CoI Couperus. Ph.D. thesis.
This will be a robust test of magnetic predictability.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-03-25T06:29:43Z/2022-03-25T11:32:38Z
Version PPS_NOT_AVAILABLE
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 2022-03-31T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2022, Fraternal Or Identicalquestionmark The Magnetic Properties Of M Dwarf Twins, PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.57780/esa-awtxc3g