Results 11 to 20 of about 10,149 (153)
Asteroseismology [PDF]
, 2012 Asteroseismology is the determination of the interior structures of stars by
using their oscillations as seismic waves. Simple explanations of the
astrophysical background and some basic theoretical considerations needed in
this rapidly evolving field ...A Baglin, A Gautschy, A Miglio, A Mukadam, AA Pamyatnykh, AB Kaye, AJ Brickhill, AU Landolt, B Mosser, C Aerts, C Aerts, C Waelkens, C Waelkens, D Kilkenny, DE Mkrtichian, DE Winget, DE Winget, DE Winget, DE Winget, DO Gough, DR Reese, DW Kurtz, DW Kurtz, DW Kurtz, EB Frost, EL Robinson, EM Green, F-L Deubner, G Handler, G Handler, G Handler, G Handler, G Maeder, G Torres, G Walker, H Bruntt, H Kjeldsen, H Saio, J Christensen-Dalsgaard, J Christensen-Dalsgaard, J Daszyńska-Daszkiewicz, J Daszyńska-Daszkiewicz, J Daszyńska-Daszkiewicz, J Goodricke, J Ridder De, J-P Montagner, JH Telting, JH Telting, JP Cox, JR Percy, L Eyer, LL Kiss, M Aizenman, M Asplund, M Suran, M Tassoul, M-A Dupret, MD Reed, MH Montgomery, MH Montgomery, N Baker, P Brassard, P Dufour, PA Woudt, PW Jones, R Samadi, RD Watson, RE Nather, RE Nather, RL Gilliland, S Frandsen, S Hekker, S Rosseland, S Talon, SO Kepler, SS Vogt, T Kallinger, TR Bedding, TR Bedding, TS Metcalfe, TS Metcalfe, WA Dziembowski, WA Dziembowski, WA Dziembowski, WA Dziembowski, WD Pesnell, WJ Chaplin, WW Campbell +87 morecore +2 more sourcesSaturn's Rings as a Seismograph to Probe Saturn's Internal Structure
AGU Advances, Volume 1, Issue 2, June 2020., 2020 As it has already done for Earth, the Sun, and the stars, seismology has the potential to radically change the way the interiors of giant planets are studied. In a sequence of events foreseen by only a few, observations of Saturn's rings by the Cassini spacecraft have rapidly broken ground on giant planet seismology. Gravity directly couples the planet'Christopher R. Mankovichwiley +1 more sourceAsteroseismology and interferometry [PDF]
The Astronomy and Astrophysics Review, 2007 Asteroseismology provides us with a unique opportunity to improve our understanding of stellar structure and evolution. Recent developments, including the first systematic studies of solar-like pulsators, have boosted the impact of this field of research within Astrophysics and have led to a significant increase in the size of the research community ...Cunha, M.S., Aerts, C., Christensen-Dalsgaard, J., Baglin, A., Bigot, Lionel, Brown, T.M., Catala, C., Creevey, O.L., Domiciano de Souza, A., Eggenberger, P., Garcia, P.J.V., Grundahl, F., Kervella, P., Kurtz, D.W., Mathias, P., Miglio, A., Monteiro, M.J.P.F.G., Perrin, G., Pijpers, F.P., Pourbaix, D., Quirrenbach, A., Rousselet-Perraut, K., Teixeira, T.C., Thévenin, F., Thompson, M.J. +24 moreopenaire +7 more sourcesTESS asteroseismology of the known red-giant host stars HD 212771 and HD 203949 [PDF]
, 2019 International ...Adibekyan, Vardan, Aguirre, Víctor Silva, Antia, H. M., Ball, Warrick, Basu, Sarbani, Bean, Jacob L., Bedding, Timothy R., Bossini, Diego, Campante, Tiago L., Chaplin, William J., Christensen-Dalsgaard, Jørgen, Corsaro, Enrico, Cunha, Margarida S., Davies, Guy R., García, Rafael A., Handberg, Rasmus, Hon, Marc, Huber, Daniel, Kane, Stephen R., Kawaler, Steven D., Kjeldsen, Hans, Kuszlewicz, James S., Lucas, Miles, Lund, Mikkel N., Mathur, Savita, Mena, Elisa Delgado, Metcalfe, Travis S., Miglio, Andrea, Monteiro, Mário J. P. F. G., Mosser, Benoît, Nardetto, Nicolas, Nielsen, Martin B., Nsamba, Benard, Pereira, Filipe, Pinsonneault, Marc H., Reffert, Sabine, Serenelli, Aldo M., Sousa, Sérgio G., Stassun, Keivan G., Stello, Dennis, Stock, Stephan, Tsantaki, Maria, Turnbull, Margaret C., Veras, Dimitri, Vrard, Mathieu, Yıldız, Mutlu, Çelik Orhan, Zeynep, Örtel, Sibel +47 morecore +5 more sourcesPLATO as it is: A legacy mission for Galactic archaeology
Astronomische Nachrichten, Volume 338, Issue 6, Page 644-661, July 2017., 2017 Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high‐resolution chrono‐chemo‐kinematical maps of the Galaxy. Data from large‐scale astrometric and spectroscopic surveys will soon provide us with a well‐defined view of the current chemo‐kinematical structure of the Milky Way, but it ...A. Miglio, C. Chiappini, B. Mosser, G. R. Davies, K. Freeman, L. Girardi, P. Jofré, D. Kawata, B. M. Rendle, M. Valentini, L. Casagrande, W. J. Chaplin, G. Gilmore, K. Hawkins, B. Holl, T. Appourchaux, K. Belkacem, D. Bossini, K. Brogaard, M.‐J. Goupil, J. Montalbán, A. Noels, F. Anders, T. Rodrigues, G. Piotto, D. Pollacco, H. Rauer, C. Allende Prieto, P. P. Avelino, C. Babusiaux, C. Barban, B. Barbuy, S. Basu, F. Baudin, O. Benomar, O. Bienaymé, J. Binney, J. Bland‐Hawthorn, A. Bressan, C. Cacciari, T. L. Campante, S. Cassisi, J. Christensen‐Dalsgaard, F. Combes, O. Creevey, M. S. Cunha, R. S. Jong, P. Laverny, S. Degl'Innocenti, S. Deheuvels, É. Depagne, J. Ridder, P. Di Matteo, M. P. Di Mauro, M.‐A. Dupret, P. Eggenberger, Y. Elsworth, B. Famaey, S. Feltzing, R. A. García, O. Gerhard, B. K. Gibson, L. Gizon, M. Haywood, R. Handberg, U. Heiter, S. Hekker, D. Huber, R. Ibata, D. Katz, S. D. Kawaler, H. Kjeldsen, D. W. Kurtz, N. Lagarde, Y. Lebreton, M. N. Lund, S. R. Majewski, P. Marigo, M. Martig, S. Mathur, I. Minchev, T. Morel, S. Ortolani, M. H. Pinsonneault, B. Plez, P. G. Prada Moroni, D. Pricopi, A. Recio‐Blanco, C. Reylé, A. Robin, I. W. Roxburgh, M. Salaris, B. X. Santiago, R. Schiavon, A. Serenelli, S. Sharma, V. Silva Aguirre, C. Soubiran, M. Steinmetz, D. Stello, K. G. Strassmeier, P. Ventura, R. Ventura, N. A. Walton, C. C. Worley +104 morewiley +1 more sourceThe Dark Side of Neutron Stars
Advances in High Energy Physics, Volume 2013, Issue 1, 2013., 2013 We review severe constraints on asymmetric bosonic dark matter based on observations of old
neutron stars. Under certain conditions, dark matter particles in the form of asymmetric bosonic
WIMPs can be effectively trapped onto nearby neutron stars, where they can rapidly thermalize and
concentrate in the core of the star.Chris Kouvaris, Konstantin Belotskywiley +1 more sourceAsteroseismology and magnetic cycles [PDF]
Astronomische Nachrichten, 2012 AbstractSmall cyclic variations in the frequencies of acoustic modes are expected to be a common phenomenon in solar‐like pulsators, as a result of stellar magnetic activity cycles. The frequency variations observed throughout the solar and stellar cycles contain information about structural changes that take place inside the stars as well as about ...Santos, A. R. G., Cunha, M. S., Lima, J. J. G. +2 moreopenaire +2 more sources