Zobrazeno 1 - 10
of 146
pro vyhledávání: '"Silva Aguirre V"'
Autor:
Campante T. L., Barclay T., Swift J. J., Huber D., Adibekyan V. Zh., Cochran W., Burke C. J., Isaacson H., Quintana E. V., Davies G. R., Silva Aguirre V., Ragozzine D., Riddle R., Baranec C., Basu S., Chaplin W. J., Christensen-Dalsgaard J., Metcalfe T. S., Bedding T. R., Handberg R., Stello D., Brewer J. M., Hekker S., Karoff C., Kolbl R., Law N. M., Lundkvist M., Miglio A., Rowe J. F., Santos N. C., Van Laerhoven C., Arentoft T., Elsworth Y. P., Fischer D. A., Kawaler S. D., Kjeldsen H., Lund M. N., Marcy G. W., Sousa S. G., Sozzetti A., White T. R.
Publikováno v:
EPJ Web of Conferences, Vol 101, p 02004 (2015)
The first discoveries of exoplanets around Sun-like stars have fueled efforts to find ever smaller worlds evocative of Earth and other terrestrial planets in the Solar System. While gas-giant planets appear to form preferentially around metal-rich st
Externí odkaz:
https://doaj.org/article/88d4a77566b74be7bc827926515b813e
Autor:
Deheuvels S., Silva Aguirre V., Cunha M. S., Appourchaux T., Ballot J., Brandão I., Lebreton Y., Michel E.
Publikováno v:
EPJ Web of Conferences, Vol 101, p 01013 (2015)
The sizes of stellar convective cores remain uncertain because of our poor understanding of the interface between convective and radiative zones. The very high precision of the seismic data provided by the CoRoT and Kepler space missions offers a gre
Externí odkaz:
https://doaj.org/article/8b6e4362d5384a9f8455e58400bfbb30
Autor:
Miglio, A., Brogaard, K., Stello, D., Chaplin, W. J., D'Antona, F., Montalban, J., Basu, S., Bressan, A., Grundahl, F., Pinsonneault, M., Serenelli, A. M., Elsworth, Y., Hekker, S., Kallinger, T., Mosser, B., Ventura, P., Bonanno, A., Noels, A., Silva-Aguirre, V., Szabo, R., Li, J., McCauliff, S., Middour, C. K., Kjeldsen, H.
Mass loss of red giant branch (RGB) stars is still poorly determined, despite its crucial role in the chemical enrichment of galaxies. Thanks to the recent detection of solar-like oscillations in G-K giants in open clusters with Kepler, we can now di
Externí odkaz:
http://arxiv.org/abs/1109.4376
Autor:
Chaplin, W. J., Lund, M. N., Handberg, R., Basu, S., Buchhave, L. A., Campante, T. L., Davies, G. R., Huber, D., Latham, D. W., Latham, C. A., Serenelli, A., Antia, H. M., Appourchaux, T., Ball, W. H., Benomar, O., Casagrande, L., Christensen-Dalsgaard, J., Coelho, H. R., Creevey, O. L., Elsworth, Y., García, R. A., Gaulme, P., Hekker, S., Kallinger, T., Karoff, C., Kawaler, S. D., Kjeldsen, H., Lundkvist, M. S., Marcadon, F., Mathur, S., Miglio, A., Mosser, B., Régulo, C., Roxburgh, I. W., Silva Aguirre, V., Stello, D., Verma, K., White, T. R., Bedding, T. R., Barclay, T., Buzasi, D. L., Dehuevels, S., Gizon, L., Houdek, G., Howell, S. B., Salabert, D., Soderblom, D. R.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2015 Oct 01. 127(956), 1038-1044.
Externí odkaz:
https://www.jstor.org/stable/10.1086/683103
Autor:
Abdurro'Uf, Accetta, K, Aerts, C, Silva Aguirre, V, Ahumada, R, Ajgaonkar, N, Filiz Ak, N, Alam, S, Allende Prieto, C, Almeida, A, Anders, F, Anderson, SF, Andrews, BH, Anguiano, B, Aquino-Ortíz, E, Aragón-Salamanca, A, Argudo-Fernández, M, Ata, M, Aubert, M, Avila-Reese, V, Badenes, C, Barbá, RH, Barger, K, Barrera-Ballesteros, JK, Beaton, RL, Beers, TC, Belfiore, F, Bender, CF, Bernardi, M, Bershady, MA, Beutler, F, Bidin, CM, Bird, JC, Bizyaev, D, Blanc, GA, Blanton, MR, Boardman, NF, Bolton, AS, Boquien, M, Borissova, J, Bovy, J, Brandt, WN, Brown, J, Brownstein, Brusa, M, Buchner, J, Bundy, K, Burchett, JN, Bureau, M, Burgasser, A, Cabang, TK, Campbell, S, Cappellari, M, Carlberg, JK, Wanderley, FC, Carrera, R, Cash, J, Chen, YP, Chen, WH, Cherinka, B, Chiappini, C, Choi, PD, Chojnowski, SD, Chung, H, Clerc, N, Cohen, RE, Comerford, JM, Comparat, J, Da Costa, L, Covey, K, Crane, JD, Cruz-Gonzalez, I, Culhane, C, Cunha, K, Dai, YS, Damke, G, Darling, J, Davidson, JW, Davies, R, Dawson, K, De Lee, N, Diamond-Stanic, AM, Cano-Díaz, M, Sánchez, HD, Donor, J, Duckworth, C, Dwelly, T, Eisenstein, DJ, Elsworth, YP, Emsellem, E, Eracleous, M, Escoffier, S, Fan, X, Farr, E, Feng, S, Fernández-Trincado, JG, Feuillet, D, Filipp, A, Fillingham, SP, Frinchaboy, PM
Publikováno v:
The Astrophysical Journal Supplement Series, vol 259, iss 2
This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete release of the Mapping Nearby Galaxies at Apache Point Observatory (M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ee51145e6cfa42494c5a5e17401e9b74
Akademický článek
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Autor:
Silva Aguirre, V., Christensen-Dalsgaard, J., Cassisi, S., Miller Bertolami, M., Serenelli, A. M., Stello, D., Weiss, A., Angelou, G., Jiang, C., Lebreton, Y., Spada, F., Bellinger, E. P., Deheuvels, S., Ouazzani, R. M., Pietrinferni, A., Mosumgaard, J. R., Townsend, R. H. D., Battich, T., Bossini, D., Constantino, T., Eggenberger, P., Hekker, S., Mazumdar, A., Miglio, A., Nielsen, K. B., Salaris, M.
Publikováno v:
Silva Aguirre, V, Christensen-Dalsgaard, J, Cassisi, S, Miller Bertolami, M, Serenelli, A M, Stello, D, Weiss, A, Angelou, G, Jiang, C, Lebreton, Y, Spada, F, Bellinger, E P, Deheuvels, S, Ouazzani, R M, Pietrinferni, A, Mosumgaard, J R, Townsend, R H D, Battich, T, Bossini, D, Constantino, T, Eggenberger, P, Hekker, S, Mazumdar, A, Miglio, A, Nielsen, K B & Salaris, M 2019 ' The Aarhus Red Giants Challenge I : Stellar structures in the red giant branch phase ' ArXiv . < https://arxiv.org/abs/1912.04909 >
(Abridged). We introduce the Aarhus Red Giants Challenge, a series of detailed comparisons between widely used stellar evolution and oscillation codes aiming at establishing the minimum level of uncertainties in properties of red giants arising solel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pure_au_____::cd0163b0a9a653d03c87f7288c5dd285
https://pure.au.dk/portal/da/publications/the-aarhus-red-giants-challenge-i(7488643a-bf68-4b05-86d9-d82fc51cb41f).html
https://pure.au.dk/portal/da/publications/the-aarhus-red-giants-challenge-i(7488643a-bf68-4b05-86d9-d82fc51cb41f).html
Stellar magnetic activity is an important parameter to study as it can give insights into stellar activity cycles and even how the stellar dynamo operates. However, as cool stars evolve along the main sequence, they lose angular momentum due to magne
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7f0093a0e50f73088f94ca113bf52b8
Publikováno v:
Astronomy & Astrophysics / Astronomie et Astrophysique; Oct2020, Vol. 642, p1-18, 18p
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Jan2020, Vol. 491 Issue 1, p455-467, 13p