Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Baruteau, Clément"'
Gas giant planets are turbulent rotating magnetic objects that have strong and complex interactions with their environment. In such systems, the dissipation of tidal waves excited by tidal forces shape the orbital architecture and the rotational dyna
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::daa2e9d4081a9e1937ede6f3b3146260
Autor:
Astoul, Aurélie, Mathis, Stéphane, Baruteau, Clément, Park, Junho, Gallet, Florian, Strugarek, Antoine, Augustson, Kyle C., Brun, Sacha A., Bolmont, Emeline
Over 4000 exoplanets have been discovered in the past 25 years or so, most of which orbit cool stars. Star-planet tidal interactions are known to drive the late evolution of the shortest-period planetary systems via tidal dissipation. Such dissipatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a16c1e6d18256775b706a3f92b9c2cb
Autor:
Astoul, Aurélie, Mathis, Stéphane, Baruteau, Clément, Gallet, Florian, Strugarek, Antoine, Augustson, Kyle, Brun, Allan Sacha, Bolmont, Emeline
Publikováno v:
Extreme Solar Systems 4
Extreme Solar Systems 4, Aug 2019, Reykjavik, Iceland
Extreme Solar Systems 4, Aug 2019, Reykjavik, Iceland
International audience; Over the last two decades, about 4000 exoplanets have been discovered around low-mass stars. For the shortest period exoplanets, star-planet tidal interactions are likely to have played a major role in the ultimate orbital evo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::d35bc2f280aedeea660235689c710b86
https://hal.archives-ouvertes.fr/hal-02370766
https://hal.archives-ouvertes.fr/hal-02370766
Autor:
Zhang, Shangjia, Zhu, Zhaohuan, Huang, Jane, Guzman, Viviana V., Andrews, Sean M., Birnstiel, Tilman, Dullemond, Cornelis P., Carpenter, John M., Isella, Andrea, Pérez, Laura M., Benisty, Myriam, Baruteau, Clément, Bai, Xue-Ning, Ricci, Luca
Publikováno v:
American Astronomical Society, AAS Meeting #233
American Astronomical Society, AAS Meeting #233, Jan 2019, Seattle, United States
American Astronomical Society, AAS Meeting #233, Jan 2019, Seattle, United States
International audience; Discoveries over the past few decades show that planets are common. However, most discovered exoplanets are mature, so their orbital properties have gone through dynamics alteration. To test planet formation theory, it is cruc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::ac69e236ac5014786cda964abcaf42b3
https://hal.archives-ouvertes.fr/hal-02370803
https://hal.archives-ouvertes.fr/hal-02370803
Publikováno v:
The 19th Cambridge Workshop on Cool Stars, Stellar systems, and the Sun
Tidal interactions in close star-planet or binary star systems may excite inertial waves (their restoring force is the Coriolis force) in the convective region of the stars. The dissipation of these waves plays a prominent role in the long-term orbit
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2012, 423 (1), pp.L65-L69. ⟨10.1111/j.1745-3933.2012.01258.x⟩
Monthly Notices of the Royal Astronomical Society: Letters, 2012, 423 (1), pp.L65-L69. ⟨10.1111/j.1745-3933.2012.01258.x⟩
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2012, 423 (1), pp.L65-L69. ⟨10.1111/j.1745-3933.2012.01258.x⟩
Monthly Notices of the Royal Astronomical Society: Letters, 2012, 423 (1), pp.L65-L69. ⟨10.1111/j.1745-3933.2012.01258.x⟩
We present two-dimensional hydrodynamical simulations of the tidal interaction between a supermassive black hole binary with moderate mass ratio, and the fossil gas disc where it is embedded. Our study extends previous one-dimensional height-integrat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_dedup_::6ef95044909edba747e8150e5c937579
https://hal.archives-ouvertes.fr/hal-02369761
https://hal.archives-ouvertes.fr/hal-02369761
Autor:
Baruteau, Clément, Masset, Frédéric
Planetary migration is the process by which a forming planet undergoes a drift of its semi-major axis caused by the tidal interaction with its parent protoplanetary disc. One of the key quantities to assess the migration of embedded planets is the ti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_______::a41a0f572ffcbaad792ea1e51092137e
http://arxiv.org/abs/1203.3294
http://arxiv.org/abs/1203.3294
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2011, 416 (3), pp.1971-1982. ⟨10.1111/j.1365-2966.2011.19172.x⟩
Monthly Notices of the Royal Astronomical Society, 2011, 416 (3), pp.1971-1982. ⟨10.1111/j.1365-2966.2011.19172.x⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2011, 416 (3), pp.1971-1982. ⟨10.1111/j.1365-2966.2011.19172.x⟩
Monthly Notices of the Royal Astronomical Society, 2011, 416 (3), pp.1971-1982. ⟨10.1111/j.1365-2966.2011.19172.x⟩
The observation of massive exoplanets at large separation from their host star, like in the HR 8799 system, challenges theories of planet formation. A possible formation mechanism involves the fragmentation of massive self-gravitating discs into clum
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::afc044bf50048b5219fa9c24f8cfe3a2
https://hal.archives-ouvertes.fr/hal-02369770
https://hal.archives-ouvertes.fr/hal-02369770