Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Régulo, Clara"'
Autor:
Huber, Daniel, Chaplin, William J., Chontos, Ashley, Kjeldsen, Hans, Christensen-Dalsgaard, Joergen, Bedding, Timothy R., Ball, Warrick, Brahm, Rafael, Espinoza, Nestor, Henning, Thomas, Jordan, Andres, Sarkis, Paula, Knudstrup, Emil, Albrecht, Simon, Grundahl, Frank, Andersen, Mads Fredslund, Palle, Pere L., Crossfield, Ian, Fulton, Benjamin, Howard, Andrew W., Isaacson, Howard T., Weiss, Lauren M., Handberg, Rasmus, Lund, Mikkel N., Serenelli, Aldo M., Mosumgaard, Jakob, Stokholm, Amalie, Bierlya, Allyson, Buchhave, Lars A., Latham, David W., Quinn, Samuel N., Gaidos, Eric, Hirano, Teruyuki, Ricker, George R., Vanderspek, Roland K., Seager, Sara, Jenkins, Jon M., Winn, Joshua N., Antia, H. M., Appourchaux, Thierry, Basu, Sarbani, Bell, Keaton J., Benomar, Othman, Bonanno, Alfio, Buzasi, Derek L., Campante, Tiago L., Orhan, Z. Celik, Corsaro, Enrico, Cunha, Margarida S., Davies, Guy R., Deheuvels, Sebastien, Grunblatt, Samuel K., Hasanzadeh, Amir, Di Mauro, Maria Pia, Garcia, Rafael A., Gaulme, Patrick, Girardi, Leo, Guzik, Joyce A., Hon, Marc, Jiang, Chen, Kallinger, Thomas, Kawaler, Steven D., Kuszlewicz, James S., Lebreton, Yveline, Li, Tanda, Lucas, Miles, Lundkvist, Mia S., Mathis, Stephane, Mathur, Savita, Mazumdar, Anwesh, Metcalfe, Travis S., Miglio, Andrea, Monteiro, Mario J., Mosser, Benoit, Noll, Anthony, Nsamba, Benard, Mann, Andrew W., Ong, Jia Mian Joel, Ortel, S., Pereira, Filipe, Ranadive, Pritesh, Regulo, Clara, Rodrigues, Thaise S., Roxburgh, Ian W., Aguirre, Victor Silva, Smalley, Barry, Schofield, Mathew, Sousa, Sergio G., Stassun, Keivan G., Stello, Dennis, Tayar, Jamie, White, Timothy R., Verma, Kuldeep, Vrard, Mathieu, Yildiz, M., Baker, David, Bazot, Michael, Beichmann, Charles, Bergmann, Christoph, Bugnet, Lisa, Cale, Bryson, Carlino, Roberto, Cartwright, Scott M., Christiansen, Jessie L., Ciardi, David R., Creevey, Orlagh, Dittmann, Jason A., Nascimento, Jose Dias Do, van Eylen, Vincent, Furesz, Gabor, Gagne, Jonathan, Gao, Peter, Gazeas, Kosmas, Giddens, Frank, Hall, Oliver, Hekker, Saskia, Ireland, Michael J., Latouf, Natasha, LeBrun, Danny, Levine, Alan M, Matzko, William, Natinsky, Eva, Page, Emma, Plavchan, Peter, Mansouri-Samani, Masoud, McCauliff, Sean, Mullally, Susan E, Orenstein, Brendan, Soto, Aylin, Paegert, Martin, van Saders, Jennifer L., Schnaible, Chloe, Soderblom, David R., Szabo, Robert, Tanner, Angelle, Tinney, C. G., Teske, Johanna, Thomas, Alexandra, Trampedach, Regner, Wright, Duncan, Yuan, Thomas T., Zohrabi, Farzaneh
We present the discovery of TOI-197.01, the first transiting planet identified by the Transiting Exoplanet Survey Satellite (TESS) for which asteroseismology of the host star is possible. TOI-197 (HIP116158) is a bright (V=8.2 mag), spectroscopically
Externí odkaz:
http://arxiv.org/abs/1901.01643
Autor:
Mathur, Savita, Garcia, Rafael A., Huber, Daniel, Regulo, Clara, Stello, Dennis, Beck, Paul G., Houmani, Kenza, Salabert, David
The Kepler mission has been a success in both exoplanet search and stellar physics studies. Red giants have actually been quite a highlight in the Kepler scene. The Kepler long and almost continuous four-year observations allowed us to detect oscilla
Externí odkaz:
http://arxiv.org/abs/1611.04237
Autor:
Gizon, Laurent, Ballot, Jérome, Michel, Eric, Stahn, Thorsten, Vauclair, Gérard, Bruntt, Hans, Quirion, Pierre-Olivier, Benomar, Othman, Vauclair, Sylvie, Appourchaux, Thierry, Auvergne, Michel, Baglin, Annie, Barban, Caroline, Baudin, Fréderic, Bazot, Michaël, Campante, Tiago, Catala, Claude, Chaplin, William, Creevey, Orlagh, Deheuvels, Sébastien, Dolez, Noël, Elsworth, Yvonne, García, Rafael, Gaulme, Patrick, Mathis, Stéphane, Mathur, Savita, Mosser, Benoît, Régulo, Clara, Roxburgh, Ian, Salabert, David, Samadi, Réza, Sato, Kumiko, Verner, Graham, Hanasoge, Shravan, Sreenivasan, Katepalli R.
Publikováno v:
PNAS 2013, vol. 110, no. 33, pp. 13267-13271
Rotation is thought to drive cyclic magnetic activity in the Sun and Sun-like stars. Stellar dynamos, however, are poorly understood owing to the scarcity of observations of rotation and magnetic fields in stars. Here, inferences are drawn on the int
Externí odkaz:
http://arxiv.org/abs/1308.4352
Autor:
Bonaca, Ana, Tanner, Joel D., Basu, Sarbani, Chaplin, William J., Metcalfe, Travis S., Monteiro, Mário J. P. F. G., Ballot, Jérôme, Bedding, Timothy R., Bonanno, Alfio, Broomhall, Anne-Marie, Bruntt, Hans, Campante, Tiago L., Christensen-Dalsgaard, Jørgen, Corsaro, Enrico, Elsworth, Yvonne, García, Rafael A., Hekker, Saskia, Karoff, Christoffer, Kjeldsen, Hans, Mathur, Savita, Régulo, Clara, Roxburgh, Ian, Stello, Dennis, Trampedach, Regner, Barclay, Thomas, Burke, Christopher J., Caldwell, Douglas A.
Stellar models generally use simple parametrizations to treat convection. The most widely used parametrization is the so-called "Mixing Length Theory" where the convective eddy sizes are described using a single number, \alpha, the mixing-length para
Externí odkaz:
http://arxiv.org/abs/1207.2765
Autor:
Howell, Steve B., Rowe, Jason F., Bryson, Stephen T., Quinn, Samuel N., Marcy, Geoffrey W., Isaacson, Howard, Ciardi, David R., Chaplin, William J., Metcalfe, Travis S., Monteiro, Mario J. P. F. G., Appourchaux, Thierry, Basu, Sarbani, Creevey, Orlagh L., Gilliland, Ronald L., Quirion, Pierre-Olivier, Stello, Denis, Kjeldsen, Hans, Christensen-Dalsgaard, Jorgen, Elsworth, Yvonne, García, Rafael A., Houdek, Gunter, Karoff, Christoffer, Molenda-Żakowicz, Joanna, Thompson, Michael J., Verner, Graham A., Torres, Guillermo, Fressin, Francois, Crepp, Justin R., Adams, Elisabeth, Dupree, Andrea, Sasselov, Dimitar D., Dressing, Courtney D., Borucki, William J., Koch, David G., Lissauer, Jack J., Latham, David W., Gautier III, Thomas N., Everett, Mark, Horch, Elliott, Batalha, Natalie M., Dunham, Edward W., Szkody, Paula, Silva, David R., Mighel, Ken, Holberg, Jay, Ballot, Jer^ome, Bedding, Timothy R., Bruntt, Hans, Campante, Tiago L., Handberg, Rasmus, Hekker, Saskia, Huber, Daniel, Mathur, Savita, Mosser, Benoit, Régulo, Clara, White, Timothy R., Christiansen, Jessie L., Middour, Christopher K., Haas, Michael R., Hall, Jennifer R., Jenkins, Jon M., McCaulif, Sean, Fanelli, Michael N., Kulesa, Craig, McCarthy, Don, Henze, Christopher E.
We present Kepler observations of the bright (V=8.3), oscillating star HD 179070. The observations show transit-like events which reveal that the star is orbited every 2.8 days by a small, 1.6 R_Earth object. Seismic studies of HD 179070 using short
Externí odkaz:
http://arxiv.org/abs/1112.2165
Autor:
White, Timothy R., Bedding, Timothy R., Stello, Dennis, Appourchaux, Thierry, Ballot, Jérôme, Benomar, Othman, Bonanno, Alfio, Broomhall, Anne-Marie, Campante, Tiago L., Chaplin, William J., Christensen-Dalsgaard, Jørgen, Corsaro, Enrico, Doğan, Gülnur, Elsworth, Yvonne P., Fletcher, Stephen T., García, Rafael A., Gaulme, Patrick, Handberg, Rasmus, Hekker, Saskia, Huber, Daniel, Karoff, Christoffer, Kjeldsen, Hans, Mathur, Savita, Mosser, Benoit, Monteiro, Mario J. P. F. G., Régulo, Clara, Salabert, David, Aguirre, Victor Silva, Thompson, Michael J., Verner, Graham, Morris, Robert L., Sanderfer, Dwight T., Seader, Shawn E.
Photometric observations made by the NASA Kepler Mission have led to a dramatic increase in the number of main-sequence and subgiant stars with detected solar-like oscillations. We present an ensemble asteroseismic analysis of 76 solar-type stars. Us
Externí odkaz:
http://arxiv.org/abs/1110.1375
Autor:
Mathur, Savita, Garcia, Rafael A., Salabert, David, Ballot, Jerome, Regulo, Clara, Metcalfe, Travis S., Baglin, Annie
It is well known that in the Sun, the frequencies and amplitudes of acoustic modes vary throughout the solar cycle. Indeed, while the magnetic activity goes towards its maximum, the frequencies of the modes increase and their amplitudes decrease. We
Externí odkaz:
http://arxiv.org/abs/1011.4102
Autor:
Garcia, Rafael A., Mathur, Savita, Salabert, David, Ballot, Jerome, Regulo, Clara, Metcalfe, Travis S., Baglin, Annie
Publikováno v:
Science.329:1032,2010
The 11-year activity cycle of the Sun is a consequence of a dynamo process occurring beneath its surface. We analyzed photometric data obtained by the CoRoT space mission, showing solar-like oscillations in the star HD49933, for signatures of stellar
Externí odkaz:
http://arxiv.org/abs/1008.4399
Akademický článek
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Publikováno v:
Proceedings of the International Astronomical Union. 05/02/2008, Vol. 4 Issue S253, p374-377. 4p.