Zobrazeno 31 - 40
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pro vyhledávání: '"Baruteau, Clément"'
Akademický článek
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Autor:
Kraus, Stefan, Monnier, John D., Ireland, Michael J., Duchene, Gaspard, Espaillat, Catherine, Hoenig, Sebastian, Juhasz, Attila, Mordasini, Chris, Olofsson, Johan, Paladini, Claudia, Stassun, Keivan, Turner, Neal, Vasisht, Gautam, Harries, Tim J., Bate, Matthew R., Gonzalez, Jean-Francois, Matter, Alexis, Zhu, Zhaohuan, Panic, Olja, Regaly, Zsolt, Morbidelli, Alessandro, Meru, Farzana, Wolf, Sebastian, Ilee, John, Berger, Jean-Philippe, Zhao, Ming, Kral, Quentin, Morlok, Andreas, Bonsor, Amy, Ciardi, David, Kane, Stephen R., Kratter, Kaitlin, Laughlin, Greg, Pepper, Joshua, Raymond, Sean, Labadie, Lucas, Nelson, Richard P., Weigelt, Gerd, Brummelaar, Theo ten, Pierens, Arnaud, Oudmaijer, Rene, Kley, Wilhelm, Pope, Benjamin, Jensen, Eric L. N., Bayo, Amelia, Smith, Michael, Boyajian, Tabetha, Quiroga-Nunez, Luis Henry, Millan-Gabet, Rafael, Chiavassa, Andrea, Gallenne, Alexandre, Reynold, Mark, de Wit, Willem-Jan, Wittkowski, Markus, Millour, Florentin, Gandhi, Poshak, Almeida, Cristina Ramos, Herrero, Almudena Alonso, Packham, Chris, Kishimoto, Makoto, Tristram, Konrad R. W., Pott, Joerg-Uwe, Surdej, Jean, Buscher, David, Haniff, Chris, Lacour, Sylvestre, Petrov, Romain, Ridgway, Steve, Tuthill, Peter, van Belle, Gerard, Armitage, Phil, Baruteau, Clement, Benisty, Myriam, Bitsch, Bertram, Paardekooper, Sijme-Jan, Pinte, Christophe, Masset, Frederic, Rosotti, Giovanni P.
The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of Extremely Large Telescopes. We make the case that a breakthrough in angular resolution imaging c
Externí odkaz:
http://arxiv.org/abs/1608.00578
The growing body of observational data on extrasolar planets and protoplanetary disks has stimulated intense research on planet formation and evolution in the past few years. The extremely diverse, sometimes unexpected physical and orbital characteri
Externí odkaz:
http://arxiv.org/abs/1604.07558
The gravito-inertial waves propagating over a shellular baroclinic flow inside a rotating spherical shell are analysed using the Boussinesq approximation. The wave properties are examined by computing paths of characteristics in the non-dissipative l
Externí odkaz:
http://arxiv.org/abs/1511.05832
Autor:
Baruteau, Clément, Zhu, Zhaohuan
We investigate the dynamics of large dust grains in massive lopsided transition discs via 2D hydrodynamical simulations including both gas and dust. Our simulations adopt a ring-like gas density profile that becomes unstable against the Rossby-wave i
Externí odkaz:
http://arxiv.org/abs/1511.03498
Autor:
Zhu, Zhaohuan, Baruteau, Clément
Motivated by lopsided structures observed in some massive transition discs, we have carried out 2D numerical simulations to study vortex structure in massive discs, including the effects of disc self-gravity and the indirect force which is due to the
Externí odkaz:
http://arxiv.org/abs/1511.03497
Publikováno v:
2015 ApJ 806 253
While recent observational progress is converging on the detection of compact regions of thermal emission due to embedded protoplanets, further theoretical predictions are needed to understand the response of a protoplanetary disk to the planet forma
Externí odkaz:
http://arxiv.org/abs/1505.03392
We propose a mechanism by which dust rings in protoplanetary disks can form and be long-lasting compared to gas rings. This involves the existence of a pressure maximum which traps dust either in between two gap-opening planets or at the outermost ga
Externí odkaz:
http://arxiv.org/abs/1411.5366
While many intermediate- and high-mass main sequence stars are rapidly and differentially rotating, the effects of rotation on oscillation modes are poorly known. In this communication we present a first study of axisymmetric gravito-inertial modes i
Externí odkaz:
http://arxiv.org/abs/1411.3559
Autor:
Baruteau, Clément
La détection récente des exoplanètes a fourni un formidable laboratoire d'expérimentation des théories de formation et d'évolution planétaire. Un résultat troublant est la proportion de planètes géantes situées plus près de leur étoile q
Externí odkaz:
http://tel.archives-ouvertes.fr/tel-00334456
http://tel.archives-ouvertes.fr/docs/00/33/44/56/PDF/PhD_CB.pdf
http://tel.archives-ouvertes.fr/docs/00/33/44/56/PDF/PhD_CB.pdf