Study of stellar activity through transit mapping of starspots

dc.contributor.authorValio A.
dc.date.accessioned2024-03-13T01:31:10Z
dc.date.available2024-03-13T01:31:10Z
dc.date.issued2010
dc.description.abstractDuring the eclipse of a planet, spots and other features on the surface of the host star may be occulted. This will cause small variations in the light curve of the star. Detailed studies of these variations during planetary transits provide a wealth of information about the starspots properties such as size, position, temperature (i.e. intensity), and magnetic field. If observation of multiple transits is available, the spots lifetime can be estimated. Moreover it may also be possible to determine the stellar rotation and whether differential rotation is present. Here, the study is performed using a method that simulates the passage of a planet (dark disk) in front of a star with multiple spots of different sizes, intensities, and positions on its surface. The data variations in the light curve of the star are fit using this method, yielding the starspots properties. Results are presented for solar-like stars, such as the active star CoRoT-2a. © International Astronomical Union 2011.
dc.description.firstpage96
dc.description.issuenumberS273
dc.description.lastpage103
dc.description.volume6
dc.identifier.doi10.1017/S1743921311015079
dc.identifier.issn1743-9213
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/37164
dc.relation.ispartofProceedings of the International Astronomical Union
dc.rightsAcesso Aberto
dc.subject.otherlanguageExoplanet
dc.subject.otherlanguagePlanetary transit
dc.subject.otherlanguageStarspots
dc.subject.otherlanguageStellar activity
dc.titleStudy of stellar activity through transit mapping of starspots
dc.typeArtigo de evento
local.scopus.citations0
local.scopus.eid2-s2.0-84882969808
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84882969808&origin=inward
Arquivos