A dataset provided by the European Space Agency

Name 074307
Title Magnetic Activity in the Lowest Mass Pre-main Sequence Stars
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743070101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743070201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743070301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743070401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743070501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743070601

DOI https://doi.org/10.5270/esa-s4w69lt
Author Mr David Principe
Description The spectral type boundary that determines which very low-mass objects will
eventually become M stars, vs. brown dwarfs, remains poorly constrained during
pre-main sequence evolution. X-ray observations of pre-main sequence M stars
offer a means to probe internal and surface stellar magnetic activity, so as to
help determine this boundary. However, even though a majority of stars in the
solar neighborhood are of mid- to late-M type, the X-ray activity of such stars
remain essentially unexplored for the important age range 10-100 Myr. We propose
to use XMM-Newton to observe 14 nearby (Dvirgul50 pc), young (age 10-40 Myr) stars of
type M3-M6, to investigate the potential decrease in X-ray luminosity for very
low-mass stars at this age.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-04-15T04:06:01Z/2014-08-21T16:34:09Z
Version 17.56_20190403_1200
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 2015-09-05T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Mr David Principe, 2015, 074307, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-s4w69lt