Results 131 to 140 of about 1,052,175 (256)
Models of Star-Planet Magnetic Interaction
, 2017 Magnetic interactions between a planet and its environment are known to lead
to phenomena such as aurorae and shocks in the solar system. The large number
of close-in exoplanets that were discovered triggered a renewed interest in
magnetic interactions ...A Kopp, A McQuillan, A Strugarek, A Strugarek, A Strugarek, A Strugarek, A Strugarek, AA Vidotto, AF Lanza, AF Lanza, AF Lanza, AF Lanza, AF Lanza, AS Brun, AS Brun, BP Miller, C Damiani, C. Zanni, CA Jones, D Staab, EJ Weber, EL Shkolnik, EP Rubenstein, F Pont, FC Adams, FM Neubauer, Ignazio Pillitteri, J Bouvier, J Llama, J Saur, J Saur, J. D. Alvarado-Gómez, JD Alvarado-Gómez, JD Turner, JD Turner, JF Donati, JM Grießmeier, JT Clarke, K Poppenhaeger, L Fossati, M Cuntz, M. L. Khodachenko, ML Goodman, MW Mengel, O Cohen, O Cohen, O Cohen, O Cohen, O. Cohen, P Figueira, P Tremblin, P Zarka, PW Cauley, Randy O. Laine, RC Fleck, RO Laine, RVE Lovelace, S Duling, S Preusse, S Preusse, S Stanley, T Matsakos, VG Merkin, WH Ip, Xianzhe Jia +64 morecore +1 more sourceWhy exomoons must be rare? [PDF]
arXiv, 2017 The problem of the search for the satellites of the exoplanets (exomoons) is
discussed recently. There are very many satellites in our Solar System. But in
contrary of our Solar system, exoplanets have significant eccentricity. In
process of planetary migration, exoplanets can cross some resonances with
following growth of their orbital eccentricity ...arxiv 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 sourceThe debris disk - terrestrial planet connection
, 2011 The eccentric orbits of the known extrasolar giant planets provide evidence
that most planet-forming environments undergo violent dynamical instabilities.Amaya Moro-Martín, Avi M. Mandell, Fogg, Franck Selsis, John C. Armstrong, Mark Booth, Mark C. Wyatt, Mayor, Philip J. Armitage, Sean N. Raymond, Zakamska +10 morecore +3 more sourcesAccretion 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 sourceThe evolution of hot Jupiters revealed by the age distribution of their host stars. [PDF]
Proc Natl Acad Sci U S A, 2023 Chen DC, Xie JW, Zhou JL, Dong S, Yang JY, Zhu W, Liu C, Huang Y, Xiang MS, Wang HF, Zheng Z, Luo AL, Zhang JH, Zhu Z. +13 moreeuropepmc +1 more sourceA Testbed for Tidal Migration: The 3D Architecture of an Eccentric Hot Jupiter HD 118203 b Accompanied by a Possibly Aligned Outer Giant Planet
The Astronomical JournalCharacterizing outer companions to hot Jupiters plays a crucial role in deciphering their origins. We present the discovery of a long-period giant planet, HD 118203 c ( ${m}_{c}={11.79}_{-0.63}^{+0.69}\ {M}_{{\rm{J}}}$ , ${a}_{c}={6.28}_{-0.11}^{+0.10 ...Jingwen Zhang, Daniel Huber, Lauren M. Weiss, Jerry W. Xuan, Jennifer A. Burt, Fei Dai, Nicholas Saunders, Erik A. Petigura, Ryan A. Rubenzahl, Joshua N. Winn, Sharon X. Wang, Judah Van Zandt, Max Brodheim, Zachary R. Claytor, Ian Crossfield, William Deich, Benjamin J. Fulton, Steven R. Gibson, Samuel Halverson, Grant M. Hill, Bradford Holden, Aaron Householder, Andrew W. Howard, Howard Isaacson, Stephen Kaye, Kyle Lanclos, Russ R. Laher, Jack Lubin, Joel Payne, Arpita Roy, Christian Schwab, Abby P. Shaum, Josh Walawender, Edward Wishnow, Sherry Yeh +34 moredoaj +1 more sourceSearching for Snapshots of Giant Exoplanet Migration
NEID, an extreme precision Doppler spectrograph on the WIYN 3.5-meter Telescope at Kitt Peak National Observatory (a partnership between Indiana University, University of Wisconsin-Madison, Pennsylvania State University, Princeton University,Purdue University, NSF’s NOIRLab, and NASA), is helping unravel the origin of hot Jupiters.openaire +2 more sources
