Stellar activity analysis of Barnard's Star: very slow rotation and evidence for long-term activity cycle

Autor: Ignasi Ribas, B. Toledo-Padrón, Jeffrey D. Crane, F. J. Aceituno, Steven S. Vogt, Jennifer Burt, Franz-Josef Hambsch, J. I. González Hernández, Steve Rau, Y. Ogmen, Susana Martín-Ruiz, B. Harris, I. Cervini, E. N. Johnson, S. Vanaverbeke, Jesús Aceituno, S. Shectman, L. Pérez, Manuel Perger, Bradford P. Holden, A. Suárez Mascareño, Rafael Rebolo, Enric Palle, Matias Diaz, Pamela Arriagada, Cristina Rodríguez-López, Víctor J. S. Béjar, Alfredo Sota, E. Rodriguez, J. L. Ortiz, John Briol, D. Montes, Marcin Kiraga, Scott G. Engle, Nicolás Morales, E. Díez Alonso, E. F. Guinan, S. V. Jeffers, F. S. Urquijo, Ansgar Reiners, Franky Dubois, M. McNeely, Johanna Teske, L. Barbieri, V. Casanova, Cliff Kotnik, Ludwig Logie, Pedro J. Amado, Juan Carlos Morales, Andreas Quirrenbach, Mikko Tuomi, J. B. P. Strachan, Jose A. Caballero, Guillem Anglada-Escudé, Javier Suso López, R. P. Butler, M. Deldem, E. Herrero, D. Rodríguez, M. J. López-González, Felipe Murgas

Publikováno v: WOS:000484349700055
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Universidad Complutense de Madrid

The search for Earth-like planets around late-type stars using ultrastable spectrographs requires a very precise characterization of the stellar activity and the magnetic cycle of the star, since these phenomena induce radial velocity (RV) signals th

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b937a1441903ea0accfd037986bada1e
http://hdl.handle.net/10651/53920