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
Autores principales: Oshagh, M., Triaud, A.H.M.J., Burdanov, A., Figueira, P., Reiners, A., Santos, N.C., Faria, J., Boue, G., Diáz, R.F., Dreizler, S., Boldt, S., Delrez, L., Ducrot, E., Gillon, M., Guzman Mesa, A., Jehin, E., Khalafinejad, S., Kohl, S., Serrano, L., Udry, S.
Formato: JOUR
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: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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