Search Results - "Casanova, V M"

Stellar activity analysis of Barnard’s Star: very slow rotation and evidence for long-term activity cycle by Toledo-Padrón, B, González Hernández, J I, Rodríguez-López, C, Suárez Mascareño, A, Rebolo, R, Butler, R P, Ribas, I, Anglada-Escudé, G, Johnson, E N, Reiners, A, Caballero, J A, Quirrenbach, A, Amado, P J, Béjar, V J S, Morales, J C, Perger, M, Jeffers, S V, Vogt, S, Teske, J, Shectman, S, Crane, J, Díaz, M, Arriagada, P, Holden, B, Burt, J, Rodríguez, E, Herrero, E, Murgas, F, Pallé, E, Morales, N, López-González, M J, Díez Alonso, E, Tuomi, M, Kiraga, M, Engle, S G, Guinan, E F, Strachan, J B P, Aceituno, F J, Aceituno, J, Casanova, V M, Martín-Ruiz, S, Montes, D, Ortiz, J L, Sota, A, Briol, J, Barbieri, L, Cervini, I, Deldem, M, Dubois, F, Hambsch, F -J, Harris, B, Kotnik, C, Logie, L, Lopez, J, McNeely, M, Ogmen, Y, Pérez, L, Rau, S, Rodríguez, D, Urquijo, F S, Vanaverbeke, S

“…Abstract The search for Earth-like planets around late-type stars using ultrastable spectrographs requires a very precise characterization of the stellar…”
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Stellar activity analysis of Barnard's Star: Very slow rotation and evidence for long-term activity cycle by Toledo-Padrón, B, Hernández, J. I. González, Rodríguez-López, C, Mascareño, A. Suárez, Rebolo, R, Butler, R. P, Ribas, I, Anglada-Escudé, G, Johnson, E. N, Reiners, A, Caballero, J. A, Quirrenbach, A, Amado, P. J, Béjar, V. J. S, Morales, J. C, Perger, M, Jeffers, S. V, Vogt, S, Teske, J, Shectman, S, Crane, J, Díaz, M, Arriagada, P, Holden, B, Burt, J, Rodríguez, E, Herrero, E, Murgas, F, Pallé, E, Morales, N, López-González, M. J, Alonso, E. Díez, Tuomi, M, Kiraga, M, Engle, S. G, Guinan, E. F, Strachan, J. B. P, Aceituno, F. J, Aceituno, J, Casanova, V. M, Martín-Ruiz, S, Montes, D, Ortiz, J. L, Sota, A, Briol, J, Barbieri, L, Cervini, I, Deldem, M, Dubois, F, Hambsch, F. -J, Harris, B, Kotnik, C, Logie, L, Lopez, J, McNeely, M, Ogmen, Y, Pérez, L, Rau, S, Rodríguez, D, Urquijo, F. S, Vanaverbeke, S

“…The search for Earth-like planets around late-type stars using ultra-stable spectrographs requires a very precise characterization of the stellar activity and…”
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The field high-amplitude SX Phe variable BL Cam: results from a multisite photometric campaign. II. Evidence of a binary - possibly triple - system by Fauvaud, S, Sareyan, J. -P, Ribas, I, Rodríguez, E, Lampens, P, Klingenberg, G, Farrell, J. A, Fumagalli, F, Simonetti, J. H, Wolf, M, Santacana, G, Zhou, A. -Y, Michel, R, Fox-Machado, L, Alvarez, M, Nava-Vega, A, López-González, M. J, Casanova, V. M, Aceituno, F. J, Scheggia, I, Rives, J. -J, Hintz, E. G, Van Cauteren, P, Helvaci, M, Yesilyaprak, C, Graham, K. A, Král, L, Kocián, R, Kučáková, H, Fauvaud, M, Granslo, B. H, Michelet, J, Nicholson, M. P, Vugnon, J. -M, Kotková, L, Truparová, K, Ulusoy, C, Yasarsoy, B, Avdibegovic, A, Blauzek, M, Kliner, J, Zasche, P, Bartošíková, S, Vilášek, M, Trondal, O, Abbeel, F. Van Den, Behrend, R, Wücher, H

“…Short-period high-amplitude pulsating stars of Population I ($\delta$ Sct stars) and II (SX Phe variables) exist in the lower part of the classical (Cepheid)…”
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