A dataset provided by the European Space Agency

Name 074170
Title Coronal activity cycles in solar analog stars
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741700301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741700401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741700501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741700601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741700701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741700801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741700901

DOI 10.5270/esa-lkaazf4
Author Dr Fabio Favata
Description We propose continuation into AO13 of the ongoing long-term program for the monitoring of coronal cycles in a sample of five solar-type stars in three stellar systems. The targets have been monitored continuously since AO1, yielding the first unambiguous evidence of cyclic behavior in the X-ray emission from the coronae of cool stars. Thanks to the long-term monitoring our program is starting to show evidence of the complex behavior of stellar cycles, with significant cycle-to-cycle variability becoming apparent. The observations requested in AO-13 will allow us to capitalize on our long-term investment of XMM-Newton observing time and to continue assembling a unique long-term data set that is likely to remain unmatched for a long time.
Publication A solar-like magnetic cycle on the mature K-dwarf 61 Cygni A (HD 201091) . Boro Saikia, S., Jeffers, S. V., et all. . A&A . 594-29 . 2016 . 2016A&A...594A..29B ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Fifteen years in the high-energy life of the solar-type star HD 81809. XMM-Newton observations of a stellar activity cycle . Orlando, S., Favata, F., et all. . A&A . 605-19 . 2017 . 2017A&A...605A..19O ,
Extrasolar planets and their hosts: A new X-ray research area . Schmitt, J. H. M. M., . AN . 338-178 . 2017 . 2017AN....338..178S ,
Deconvolving the HD 81809 Binary: Rotational and Activity Evidence for a Subgiant with a Sun-like Cycle . Egeland, Ricky, . ApJ . 866-80 . 2018 . 2018ApJ...866...80E ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-04-28T00:30:53Z/2015-04-30T17:55:17Z
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 2016-05-18T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016-05-18T22:00:00Z, 074170, 17.56_20190403_1200. https://doi.org/10.5270/esa-lkaazf4