Activity induced variation in spin-orbit angles as derived from Rossiter-McLaughlin measurements

One of the most powerful methods used to estimate sky-projected spin-orbit angles of exoplanetary systems is through a spectroscopic transit observation known as the RossiterMcLaughlin (RM) effect. So far mostly single RM observations have been used to estimate the spin-orbit angle, and thus there h...

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Detalles Bibliográficos
Publicado:	2018
Materias:	Planets and satellites: Detection Planets and satellites: Fundamental parameters Stars: Activity Starspots Techniques: Photometric Techniques: Radial velocities Astrophysics Photometry Planets Satellites Stars Planets and satellites: detections Planets and satellites: fundamental parameters Stars: activity Techniques: photometric Techniques: radial velocities Orbits
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v619_n_p_Oshagh http://hdl.handle.net/20.500.12110/paper_00046361_v619_n_p_Oshagh
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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