Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Philippe Thébault"'
Autor:
Johan Olofsson, Philippe Thébault, Quentin Kral, Amelia Bayo, Anthony Boccaletti, Nicolás Godoy, Thomas Henning, Rob G van Holstein, Karina Maucó, Julien Milli, Matías Montesinos, Hanno Rein, Antranik A Sefilian
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 513:713-734
The vertical structure of debris disks provides clues about their dynamical evolution and the collision rate of the unseen planetesimals. Thanks to the ever-increasing angular resolution of contemporary instruments and facilities, we are beginning to
Autor:
Clément Perrot, Johan Olofsson, Quentin Kral, Philippe Thébault, Matías Montesinos, Grant Kennedy, Amelia Bayo, Daniela Iglesias, Rob van Holstein, Christophe Pinte
Debris disks are the signposts of collisionally eroding planetesimal circumstellar belts, whose study can put important constraints on the structure of extrasolar planetary systems. The best constraints on the morphology of disks are often obtained f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ff7424eaf6a8c86d6d67f0f339b75b0
Autor:
Francois Menard, Christian Ginski, Antonio Garufi, P. Rabou, F. Madec, Judit Szulágyi, Th. Henning, Gesa H. M. Bertrang, Philippe Feautrier, Christophe Pinte, M. Villenave, Wilhelm Kley, Giuseppe Lodato, S. Brown Sevilla, Markus Janson, Carsten Dominik, Maud Langlois, Anne-Lise Maire, Francois Wildi, Myriam Benisty, R. van Boekel, Mariangela Bonavita, Miriam Keppler, Tomas Stolker, Anna B. T. Penzlin, J. de Boer, Anthony Boccaletti, Gael Chauvin, Wolfgang Brandner, Philippe Thébault, R. G. van Holstein, Eric Pantin, Alice Zurlo, M. Feldt
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 639, pp.A62. ⟨10.1051/0004-6361/202038032⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A62. ⟨10.1051/0004-6361/202038032⟩
Astronomy & Astrophysics, 639
Astronomy & Astrophysics, 639, A62. EDP SCIENCES S A
Astronomy & Astrophysics, 639:A62. EDP Sciences
Astronomy and Astrophysics-A&A, 2020, 639, pp.A62. ⟨10.1051/0004-6361/202038032⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A62. ⟨10.1051/0004-6361/202038032⟩
Astronomy & Astrophysics, 639
Astronomy & Astrophysics, 639, A62. EDP SCIENCES S A
Astronomy & Astrophysics, 639:A62. EDP Sciences
Context. A large portion of stars is found to be part of binary or higher-order multiple systems. The ubiquity of planets found around single stars raises the question of whether and how planets in binary systems form. Protoplanetary disks are the bi
Autor:
Arthur Vigan, H. M. Schmid, N. Pawellek, Th. Henning, Anthony Cheetham, D. Gisler, Gael Chauvin, Mickael Bonnefoy, A-M. Lagrange, Q. Kral, Faustine Cantalloube, E. L. Rickman, Alice Zurlo, Julien Milli, S. Hunziker, N. Engler, S. Petrus, A. Boccaletti, O. Moeller-Nilsson, Philippe Thébault, M. Carle, C. Lazzoni, Silvano Desidera, Sascha P. Quanz, Markus Feldt, Maud Langlois, Michael R. Meyer, Raffaele Gratton, Francois Wildi, Johan Olofsson, Cyril Petit, Eric Stadler, Samantha Brown, Dino Mesa, Tomas Stolker, Christian Ginski, T. Buey
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A19. ⟨10.1051/0004-6361/201936828⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A19. ⟨10.1051/0004-6361/201936828⟩
Astronomy & Astrophysics, 635. EDP SCIENCES S A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A19. ⟨10.1051/0004-6361/201936828⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A19. ⟨10.1051/0004-6361/201936828⟩
Astronomy & Astrophysics, 635. EDP SCIENCES S A
We performed observations of the Sco-Cen F star HD 117214 aiming at a search for planetary companions and the characterization of the debris disk structure. HD 117214 was observed with the SPHERE subsystems IRDIS, IFS and ZIMPOL at optical and near-I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47bb4dd3774d32b87ce82b687c0e8635
https://hal.science/hal-02899007/file/aa36828-19.pdf
https://hal.science/hal-02899007/file/aa36828-19.pdf
Autor:
R. Roelfsema, Julien Milli, Christophe Pinte, Quentin Kral, Gael Chauvin, Jean-Charles Augereau, Thibaut Moulin, Alice Zurlo, O. Moeller-Nilsson, H. M. Schmid, C. Perrot, N. Engler, François Ménard, Philippe Thébault, A. M. Lagrange, Andreas Bazzon, Jean-Luc Beuzit, Anthony Boccaletti, Johan Olofsson, D. Mouillet, Henning Avenhaus, M. Llored, Elodie Choquet, J. Pragt, Carsten Dominik, Th. Henning
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 626, pp.A54. ⟨10.1051/0004-6361/201935363⟩
Astronomy and Astrophysics
Astronomy & Astrophysics, 626:A54. EDP Sciences
Astronomy and Astrophysics-A&A, 2019, 626, pp.A54. ⟨10.1051/0004-6361/201935363⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 626, pp.A54. ⟨10.1051/0004-6361/201935363⟩
Astronomy and Astrophysics
Astronomy & Astrophysics, 626:A54. EDP Sciences
Astronomy and Astrophysics-A&A, 2019, 626, pp.A54. ⟨10.1051/0004-6361/201935363⟩
The scattering properties of the dust originating from debris discs are still poorly known. The analysis of scattered light is however a powerful remote-sensing tool to understand the physical properties of dust particles orbiting other stars. Scatte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d0d65ce49a9a803f024984256928c838
https://hal.archives-ouvertes.fr/hal-02489267
https://hal.archives-ouvertes.fr/hal-02489267
Autor:
Quentin Kral, Francois Menard, Ágnes Kóspál, Péter Ábrahám, Thomas Henning, N. Pawellek, Attila Moór, Philippe Thébault, Johan Olofsson, Anthony Boccaletti, Alice Zurlo, Miriam Keppler, Maud Langlois, Elodie Choquet, Julien Milli, Eve J. Lee, N. Engler, Adriana Pohl, G. Chauvin, Jean-Charles Augereau
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 488 (3), pp.3507-3525. ⟨10.1093/mnras/stz1971⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 488 (3), pp.3507-3525. ⟨10.1093/mnras/stz1971⟩
Monthly Notices of the Royal Astronomical Society, 2019, 488 (3), pp.3507-3525. ⟨10.1093/mnras/stz1971⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 488 (3), pp.3507-3525. ⟨10.1093/mnras/stz1971⟩
In a multi-wavelength study of thermal emission and scattered light images we analyse the dust properties and structure of the debris disc around the A1-type main sequence star 49~Cet. As a basis for this study, we present new scattered light images
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c7a0d7982336cfe40c3c82d91ad34fb1
Autor:
Amaury H. M. J. Triaud, Mark C. Wyatt, Oliver Shorttle, Philippe Thébault, Quentin Kral, Sebastian Marino
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, 2018, 479 (2), pp.2649-2672. ⟨10.1093/mnras/sty1677⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 479 (2), pp.2649-2672. ⟨10.1093/mnras/sty1677⟩
The TRAPPIST-1 system is unique in that it has a chain of seven terrestrial Earth-like planets located close to or in its habitable zone. In this paper, we study the effect of potential cometary impacts on the TRAPPIST-1 planets and how they would af
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1178d6864c9cc668af8dafdea75b6f0c
http://arxiv.org/abs/1802.05034
http://arxiv.org/abs/1802.05034
Autor:
Anne-Lise Maire, Hervé Beust, Anne-Marie Lagrange, Daniel Rouan, D. Perret, Stéphane Udry, Miriam Keppler, S. Daemgen, Michael Meyer, M. Feldt, Arthur Vigan, D. Maurel, Thomas Henning, L. Rodet, R. G. Gratton, J. C. Augereau, Hubert Klahr, C. Petit, Johan Olofsson, A. Delboulbe, Philippe Thébault, Silvano Desidera, R. Ligi, Maud Langlois, Wolfgang Brandner, Faustine Cantalloube, Valentina D'Orazi, A. Roux, Mickael Bonnefoy, Jose Ramos, Thibaut Moulin, L. Abe, Janis Hagelberg, L. Weber, Dino Mesa, M. Carle, H. Le Coroller, Anthony Boccaletti, Matthias Samland, A. Zurlo, Raphaël Galicher, A. Pavlov, Philippe Feautrier, Markus Janson, T. Schmidt, Yves Magnard, C. Lazzoni, Gael Chauvin, F. Rigal
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 615
Astronomy and Astrophysics-A&A, 2018, 615, pp.1-13. ⟨10.1051/0004-6361/201732476⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 615, pp.1-13. ⟨10.1051/0004-6361/201732476⟩
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 615
Astronomy and Astrophysics-A&A, 2018, 615, pp.1-13. ⟨10.1051/0004-6361/201732476⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 615, pp.1-13. ⟨10.1051/0004-6361/201732476⟩
Astronomy and Astrophysics
Context. A low-mass brown dwarf has been recently imaged around HR 2562 (HD 50571), a star hosting a debris disk resolved in the far infrared. Interestingly, the companion location is compatible with an orbit coplanar with the disk and interior to th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7076aaf8e4b1f206b25ef70bcc2383d8
https://hal.archives-ouvertes.fr/hal-03732639
https://hal.archives-ouvertes.fr/hal-03732639
Autor:
P. Rabou, Matías Montesinos, A. Bayo, Julien Milli, Th. Henning, Markus Janson, N. Pawellek, Juan Carlos Beamin, C. Zamora, Jean-Charles Augereau, F. Madec, Alice Zurlo, Quentin Kral, Arnaud Sevin, Marcel Carbillet, Grant M. Kennedy, Thierry Fusco, Johan Olofsson, D. P. Iglesias, Philippe Feautrier, Philippe Thébault, Matthias R. Schreiber, François Ménard, Judit Szulágyi
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 630, pp.A142. ⟨10.1051/0004-6361/201935998⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 630, pp.A142. ⟨10.1051/0004-6361/201935998⟩
Debris disks are the natural by-products of the planet formation process. Scattered or polarized light observations are mostly sensitive to small dust grains that are released from the grinding down of bigger planetesimals. High angular resolution ob
Autor:
Francois Menard, Maud Langlois, Markus Janson, R. G. van Holstein, R. G. Gratton, Philippe Feautrier, Claudio Caceres, Wolfgang Brandner, D. Mawet, Graeme Salter, Th. Henning, E. Sissa, Amelia Bayo, Dino Mesa, M. Feldt, A. Roux, A. Pavlov, C. A. Grady, Gael Chauvin, Silvano Desidera, C. Perrot, David Mouillet, J. Lannier, Ch. Ginski, Philippe Thébault, Johan Olofsson, Thibaut Moulin, A-L. Maire, D. Le Mignant, A-M. Lagrange, T. Schmidt, Matthias R. Schreiber, C. Lazzoni, R. Ligi, Julien Milli, N. Godoy, C. Thalmann, Stephen Durkan, P. Rabou, Janis Hagelberg, Christophe Pinte, Quentin Kral, Anthony Boccaletti, L. Abe, Esther Buenzli, N. Engler, Hector Canovas, Arthur Vigan, Gérard Rousset, J. C. Augereau, Joshua E. Schlieder, S. Peretti, Ruben Asensio-Torres, Mickael Bonnefoy
Publikováno v:
Astronomy and Astrophysics
Astronomy and Astrophysics, 617, A109
Astronomy and Astrophysics, 617, A109
Context. Debris disks are the intrinsic by-products of the star and planet formation processes. Most likely due to instrumental limitations and their natural faintness, little is known about debris disks around low mass stars, especially when it come