Effects of stellar surface inhomogeneities on astrometric accuracy
Surface brightness asymmetries are a very common feature of stars. Among other effects they cause a difference between the projected centre of mass and the photocentre. The evolution of those surface features makes this difference time-dependent. In some cases the displacement can be a non-negligibl...
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Format: | Doctoral Thesis |
Language: | fr |
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Universite Libre de Bruxelles
2011
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Online Access: | http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/209872 |