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From CoRoT 102899501 to the Sun. A time evolution model of chromospheric activity on the main sequence

Eigmüller, P (2012) From CoRoT 102899501 to the Sun. A time evolution model of chromospheric activity on the main sequence. Astronomy and Astrophysics, 548, A15. EDP Sciences. DOI: 10.1051/0004-6361/201219101 ISSN 0004-6361

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Item URL in elib:https://elib.dlr.de/79518/
Document Type:Article
Title:From CoRoT 102899501 to the Sun. A time evolution model of chromospheric activity on the main sequence
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Eigmüller, Pphilipp.eigmueller (at) dlr.deUNSPECIFIED
Date:2012
Journal or Publication Title:Astronomy and Astrophysics
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
Volume:548
DOI :10.1051/0004-6361/201219101
Page Range:A15
Publisher:EDP Sciences
ISSN:0004-6361
Status:Published
Keywords:stars: activity – stars: atmospheres – stars: late-type – stars: magnetic fields – stars: rotation – starspots
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Science and Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Erforschung des Weltraums
DLR - Research theme (Project):R - Projekt COROT Beteiligung
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Extrasolar Planets and Atmospheres
Deposited By: Stiebeler, Ulrike
Deposited On:11 Dec 2012 13:32
Last Modified:19 Jul 2016 17:29

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