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pro vyhledávání: '"Zechmeister, Mathias"'
Autor:
Lafarga, Marina, Ribas, Ignasi, Reiners, Ansgar, Quirrenbach, Andreas, Amado, Pedro J., Caballero, Jose A., Azzaro, Marco, Béjar, Víctor J. S., Cortés-Contreras, Miriam, Dreizler, Stefan, Hatzes, Artie P., Henning, Thomas, Jeffers, Sandra V., Kaminski, A., Kürster, Martin, Montes, David, Morales, Juan Carlos, Oshagh, Mahmoud, Rodríguez-López, Cristina, Schöfer, Patrick, Schweitzer, Andreas, Zechmeister, Mathias
Stellar activity poses one of the main obstacles for the detection and characterisation of exoplanets around cool stars, as it can induce radial velocity (RV) signals that can hide or mimic the presence of companions. Several activity indicators are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0860eeefcc41722e9ea6f587a1f008b7
Autor:
Lafarga, Marina, Ribas, Ignasi, Reiners, Ansgar, Quirrenbach, Andreas, Amado, Pedro J., Caballero, Jose A., Azzaro, Marco, Béjar, Víctor J. S., Cortés-Contreras, Miriam, Dreizler, Stefan, Hatzes, Artie P., Henning, Thomas, Jeffers, Sandra V., Kaminski, A., Kürster, Martin, Montes, David, Morales, Juan Carlos, Oshagh, Mahmoud, Rodríguez-López, Cristina, Schöfer, Patrick, Schweitzer, Andreas, Zechmeister, Mathias
Despite stellar magnetic activity being present in most cool stars, its effects on spectroscopic observations are still not well understood. Several activity indicators are routinely used to identify activity-related signals in radial velocity (RV) m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f7dd39cdbea18d5e3c3a734f63971b5
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