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Date: 2015
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/1066683
Description: Context. Young, close stars are ideal targets for searching planets using the direct imaging technique. The determination of stellar parameters is crucial for the interpretation of imaging survey resu ... More
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Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/262351
Description: Context. As is the case for all techniques involved in the research for exoplanets, direct imaging has to take into account the probability of so-called astrophysical false positives, which are phenom ... More
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Reviewed: Reviewed
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/205052
Description: We present stellar parameters and abundances of 11 elements (Li, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni and Zn) of 13 F6-K2 main-sequence stars in the young groups AB Doradus, Carina Near and Ursa Major. ... More
Reviewed: Reviewed
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/181772
Description: Recently, several studies have shown that young, open clusters are characterized by a considerable overabundance in their barium content. In particular, D'Orazi et al. reported that in some younger cl ... More
Reviewed: Reviewed
Date: 2011
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/299682
Description: Context. The Taurus-Auriga association is perhaps the most famous prototype of a low-mass star forming region, surveyed at almost all wavelengths. Unfortunately, like several other young clusters/asso ... More
Reviewed: Reviewed
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137607
Description: We report on the ground-based follow-up program of spectroscopic and photometric observations of solar-like asteroseismic targets for the Kepler space mission. These stars constitute a large group of ... More
Reviewed: Reviewed
Authors: Chaplin, W. J | Appourchaux, T | Brown, T. M | Aguirre, V. S | Stevens, I. R | Suárez, J. C | Suran, M. D | Trampedach, R | Turck-Chièze, S | Uytterhoeven, K | Ventura, R | Wilson, P. A | Christensen-Dalsgaard, J | Gilliland, R. L | Kjeldsen, H | Borucki, W. J | Koch, D | Jenkins, J. M | Ballot, J | Basu, S | Bazot, M | Elsworth, Y | Bedding, T. R | Benomar, O | Bonanno, A | Brandão, I. M | Bruntt, H | Campante, T. L | Creevey, O. L | Mauro, M. P. Di | Doğan, G | Dreizler, S | García, R. A | Eggenberger, P | Esch, L | Fletcher, S. T | Frandsen, S | Gai, N | Gaulme, P | Handberg, R | Hekker, S | Howe, R | Huber, D | Houdek, G | Korzennik, S. G | Lebrun, J. C | Leccia, S | Martic, M | Mathur, S | Mosser, B | New, R | Quirion, P.-O | Régulo, C | Roxburgh, I. W | Karoff, C | Salabert, D | Schou, J | Sousa, S. G | Stello, D | Verner, G. A | Arentoft, T | Barban, C | Belkacem, K | Benatti, S | Biazzo, K | Metcalfe, T. S | Boumier, P | Bradley, P. A | Broomhall, A.-M | Buzasi, D. L | Claudi, R. U | Cunha, M. S | D'Antona, F | Deheuvels, S | Derekas, A | Hernández, A. García | Molenda-Żakowicz, J | Giampapa, M. S | Goupil, M. J | Gruberbauer, M | Guzik, J. A | Hale, S. J | Ireland, M. J | Kiss, L. L | Kitiashvili, I. N | Kolenberg, K | Korhonen, H | Monteiro, M. J. P. F. G | Kosovichev, A. G | Kupka, F | Lebreton, Y | Leroy, B | Ludwig, H.-G | Mathis, S | Michel, E | Miglio, A | Montalbán, J | Moya, A | Thompson, M. J | Noels, A | Noyes, R. W | Pallé, P. L | Piau, L | Preston, H. L | Cortés, T. Roca | Roth, M | Sato, K. H | Schmitt, J | Serenelli, A. M
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/137906
Description: We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5days of science operations, reveal high signal-to-nois ... More
Reviewed: Reviewed
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