Results 31 to 40 of about 3,427 (167)
Super-Earths: A New Class of Planetary Bodies
, 2011 Super-Earths, a class of planetary bodies with masses ranging from a few
Earth-masses to slightly smaller than Uranus, have recently found a special
place in the exoplanetary science.Armitage P. J., Christensen U. R., Clubb K., Dobrovolskis A. R., Fogg M. J., Ford E.B., Goldreich P., Haghighipour N., Haghighipour N., Hatzes A.P., Heng K., Michael S., Nader Haghighipour, Safronov V. S., Smoluchowski M. V., Sotin C., Stamenkovic V., Stamenkovic V., Steffen J. H., Swift D. C., Tackley P. J., Weidenschilling S. J. +21 morecore +1 more sourceTwo New Candidate Planets in Eccentric Orbits [PDF]
, 1999 Doppler measurements of two G-type main-sequence stars, HD210277 and
HD168443, reveal Keplerian variations that imply the presence of companions
with masses (M sin i) of 1.28 and 5.04 M_Jup and orbital periods of 437 d and
58 d, respectively.Bertelli G., Black D. C., de la Fuente Marcos C., Debra Fischer, Delfosse X., Duquennoy A., Favata F., Fuhrmann K., Geoffrey W. Marcy, Gonzalez G., Meyer C., Michael C. Liu, Ng Y. K., Perryman M. A. C., R. Paul Butler, Steven S. Vogt, Vogt S. S. +16 morecore +4 more sourcesThe role of the initial surface density profiles of the disc on giant
planet formation: comparing with observations [PDF]
, 2003 In order to explain the main characteristics of the observed population of
extrasolar planets and the giant planets in the Solar System, we need to get a
clear understanding of which are the initial conditions that allowed their
formation. To this end we Y. Miguel, O. M. Guilera, A. Brunini, Alexander, Alexander, Andrews, Benvenuto, Bodenheimer, Chambers, Clarke, Edgeworth, Fortier, Fortier, Goldreich, Guilera, Haisch, Hartmann, Hayashi, Hillenbrand, Hollenbach, Ida, Ida, Ikoma, Isella, Kokubo, Kuiper, Lammer, Lin, Lin, Lodders, Lynden-Bell, Lyra, Masset, Matsumura, Menou, Miguel, Miguel, Miguel, Mizuno, Mizuno, Mordasini, Nelson, Paardekooper, Safronov, Stevenson, Tanaka, Terquem, Thommes, Toomre, Triaud, Vinkovic, Weidenschilling +51 morecore +5 more sourcesThe Formation and Dynamics of Super-Earth Planets
, 2013 Super-Earths, objects slightly larger than Earth and slightly smaller than
Uranus, have found a special place in exoplanetary science. As a new class of
planetary bodies, these objects have challenged models of planet formation at
both ends of the ...Haghighipour, Nadercore +1 more sourceDetection and Characterization of Extrasolar Planets through Doppler
Spectroscopy
, 2009 Over 300 extrasolar planets have been found since 1992, showing that
planetary systems are common and exhibit an outstanding variety of
characteristics.A. Eggenberger, Adams, Agol, Alibert, Alibert, Alonso, Armitage, Bakos, Baraffe, Baranne, Barge, Barman, Barman, Barnes, Basri, Beaulieu, Beichman, Benz, Bodenheimer, Bonfils, Bonfils, Boss, Bouchy, Bouchy, Bouchy, Bouchy, Bouchy, Broeg, Brown, Brown, Brown, Brunini, Burrows, Burrows, Burrows, Butler, Butler, Butler, Butler, Cameron, Campbell, Campbell, Casertano, Charbonneau, Charbonneau, Charbonneau, Charbonneau, Chiang, Connes, Cowan, Cumming, Cumming, D'Odorico, da Silva, Delfosse, Deming, Deming, Demory, Desidera, Desort, Duquennoy, Eggenberger, Ehrenreich, Endl, Endl, Endl, Endl, Fabrycky, Fischer, Fischer, Fischer, Fischer, Ford, Ford, Fortney, Fortney, Fortney, Frink, Galland, Gaudi, Gillon, Gillon, Gonzalez, Griffin, Grillmair, Gu, Guillot, Halbwachs, Harrington, Hatzes, Henry, Ida, Ida, Ida, Ikoma, Israelian, Johnson, Johnson, Jones, Jorissen, Kasting, Kennedy, Kley, Kley, Knutson, Knutson, Konacki, Kuchner, Laughlin, Lee, Lin, Livio, Loeillet, Lovis, Lovis, Lovis, Marcy, Marcy, Marcy, Marcy, Marcy, Martín, Mayor, Mayor, Mayor, Mazeh, McArthur, McCullough, Murray, Nagasawa, Niedzielski, Noyes, Pasquini, Pasquini, Paulson, Pepe, Pepe, Pepe, Pepe, Perrier, Pinotti, Pinsonneault, Pont, Pont, Pont, Pätzold, Queloz, Queloz, Raghavan, Rasio, Redfield, Rivera, S. Udry, Saar, Saar, Santos, Santos, Santos, Santos, Santos, Santos, Sartoretti, Sato, Seager, Seager, Selsis, Setiawan, Sozzetti, Stepinski, Swain, Takeda, Tamuz, Tinetti, Tinney, Trilling, Udalski, Udalski, Udalski, Udalski, Udry, Udry, Udry, Udry, Valenti, Vidal-Madjar, Vidal-Madjar, von Bloh, Wittenmyer, Wolszczan, Wright, Wright, Wright, Wu, Zucker, Zucker, Zucker +195 morecore +2 more sourcesTESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars
The Astronomical Journal, 2023 The fate of planets around rapidly evolving stars is not well understood. Previous studies have suggested that, relative to the main-sequence population, planets transiting evolved stars ( P < 100 days) tend to have more eccentric orbits. Here we present Samuel K. Grunblatt, Nicholas Saunders, Ashley Chontos, Soichiro Hattori, Dimitri Veras, Daniel Huber, Ruth Angus, Malena Rice, Katelyn Breivik, Sarah Blunt, Steven Giacalone, Jack Lubin, Howard Isaacson, Andrew W. Howard, David R. Ciardi, Boris S. Safonov, Ivan A. Strakhov, David W. Latham, Allyson Bieryla, George R. Ricker, Jon M. Jenkins, Peter Tenenbaum, Avi Shporer, Edward H. Morgan, Veselin Kostov, Hugh P. Osborn, Diana Dragomir, Sara Seager, Roland K. Vanderspek, Joshua N. Winn +29 moredoaj +1 more sourceAccretion of Planetary Material onto Host Stars
, 2017 Accretion of planetary material onto host stars may occur throughout a star's
life. Especially prone to accretion, extrasolar planets in short-period orbits,
while relatively rare, constitute a significant fraction of the known
population, and these ...A Koenigl, A McQuillan, A Skumanich, A. Bonsor, A. P. Showman, Alexander J. Mustill, Avi M. Mandell, B Paczyński, B Zuckerman, B. D. Metzger, B. Levrard, Bill Paxton, BJR Davidsson, BMS Hansen, Brian Jackson, Brian Jackson, Brian Jackson, Brian Jackson, CC Counselman III, CD Murray, Christa Van Laerhoven, Claudia Aguilera-Gómez, D Lai, D. E. Trilling, D. Huber, D. J. A. Brown, DA Fischer, Daniel C. Fabrycky, DC Richardson, Dimitri Veras, DNC Lin, DNC Lin, Elisabeth R. Adams, Eric B. Ford, Eunkyu Han, Eva Villaver, Eva Villaver, FA Rasio, Francesca Valsecchi, Francesca Valsecchi, G Wallerstein, Gordon I. Ogilvie, H Ritter, I Ramírez, IJ Sackmann, J Irwin, J Meléndez, J. Farihi, J. H. Steffen, J. Lillo-Box, J. Nordhaus, J. Setiawan, James Guillochon, JB Alexander, JE Chambers, JK Carlberg, John H. Debes, Joleen K. Carlberg, Joshua N. Winn, JR Stauffer, Julian C. van Eyken, K Batygin, Kaloyan Penev, Kevin C. Schlaufman, L Siess, L Siess, Lauren M. Weiss, M Deal, M Jura, M. Kunitomo, M. Livio, M. Nagasawa, Marcelo Tucci Maia, NA Drake, P Chayer, P Goldreich, P Goldreich, Pin‐Gao Gu, PP Eggleton, RA Mardling, Roberto Sanchis-Ojeda, Roberto Sanchis-Ojeda, S Barnes, S Teitler, Saul Rappaport, SD Kawaler, Shang-Fei Liu, Shi Jia, Simon Albrecht, Smadar Naoz, Soko Matsumura, Sourav Chatterjee, Sylvie Théado, Sylvio Ferraz-Mello, William D. Cochran, Z Kopal +95 morecore +1 more source