A dataset provided by the European Space Agency

Name 020195
Title AN X-RAY STUDY OF A COMPLETE SAMPLE OF LATE-TYPE GIANTS WITHIN 35 PC
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201950201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201950301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201950501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201950601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201950801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201950901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201951001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201951201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201951601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201951701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201951801
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201951901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201952101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201952201

DOI https://doi.org/10.5270/esa-l7uie37
Author European Space Agency
Description We propose to observe 16 nearby late-type giants in order to perform a study of
a complete volume-limited sample of single late-type giants within 35 pc. Deep
EPIC pn observations will yield detections and X-ray fluxes at solar activity
level, which is the minimum yet observed in such stars. Substancial constraints
are expected towards our understanding of issues like the evolution of stellar
activity in post main-sequence phases, the mechanisms of dynamo action in giant
stars, and the scatter of activity in stars of similar properties and
evolutionary stage.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-01-16T04:59:39Z/2005-03-31T07:07:33Z
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 2008-08-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008, An X-Ray Study Of A Complete Sample Of Late-Type Giants Within 35 Pc, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-l7uie37