A dataset provided by the European Space Agency

Proposal ID 014363
Title Activity cycles and Maunder minima stars
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DOI https://doi.org/10.5270/esa-c9a9rrt
Principal Investigator, PI Prof Juergen Schmitt
Abstract We propose to continue monitoring three fields containing a total of fivelate-type stars for long-term variability. The stars are 61 Cyg A and B, HD 81809, all of which are being monitored for Ca emission, with 61 Cyg A andHD 81809 having cyclic activity changes, and Alpha Cen A and B, the nearestsolar-like star. All of these stars are known X-ray sources, which have alreadybenn monitored in XMM-Newton AO1. The overall goal of this series ofobservations is to obtain a baseline of a decade for these objects in order tocheck whether other solar -like stars show cyclic changes in their X-ray outputjust like the Sun.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-11-22T05:33:21Z/2005-08-17T20:34:06Z
Version 17.56_20190403_1200
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 2007-12-16T00:00:00Z
Last Update 2025-01-27
Keywords "cyclic activity", "xmm newton ao1", "hd 81809", "activity cycles", "late type stars", "XMM-Newton", "term variability", "xray output", "xray sources", "ca emission", "alpha cen", "XMM", "benn monitored", "maunder minima stars"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Juergen Schmitt, 2007, 'Activity cycles and Maunder minima stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-c9a9rrt