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Browsing by Author "Cantalloube, F."

Browsing by Author "Cantalloube, F."

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  • Direct confirmation of the radial-velocity planet ß Pictoris c 
    Nowak, M.; Lacour, S.; Lagrange, A. -M; Rubini, P.; Wang, J.; Stolker, T.; Abuter, R.; Amorim, A.; Asensio-Torres, R.; Bauböck, M.; Benisty, M.; Berger, J. P.; Beust, H.; Blunt, S.; Boccaletti, A.; Bonnefoy, M.; Bonnet, H.; Brandner, W.; Cantalloube, F.; Charnay, B.; Choquet, E.; Christiaens, V.; Clénet, Y.; Coudé Du Foresto, V.; Cridland, A.; de Zeeuw, P. T.; Dembet, R.; Dexter, J.; Drescher, A.; Duvert, G.; Eckart, A.; Eisenhauer, F.; Gao, F.; Garcia, P.; Garcia Lopez, R.; Gardner, T.; Gendron, E.; Genzel, R.; Gillessen, S.; Girard, J.; Grandjean, A.; Haubois, X.; Heißel, G.; Henning, T.; Hinkley, S.; Hippler, S.; Horrobin, M.; Houllé, M.; Hubert, Z.; Jiménez-Rosales, A.; Jocou, L.; Kammerer, J.; Kervella, P.; Keppler, M.; Kreidberg, Laura; Kulikauskas, M.; Lapeyrère, V.; Le Bouquin, J. -B; Léna, P.; Mérand, A.; Maire, A. -L; Mollière, P.; Monnier, J. D.; Mouillet, D.; Müller, A.; Nasedkin, E.; Ott, T.; Otten, G.; Paumard, T.; Paladini, C.; Perraut, K.; Perrin, G.; Pueyo, L.; Pfuhl, O.; Rameau, J.; Rodet, L.; Rodríguez-Coira, G.; Rousset, G.; Scheithauer, S.; Shangguan, J.; Stadler, J.; Straub, O.; Straubmeier, C.; Sturm, E.; Tacconi, L. J.; van Dishoeck, E. F.; Vigan, A.; Vincent, F.; von Fellenberg, S. D.; Ward-Duong, K.; Widmann, F.; Wieprecht, E.; Wiezorrek, E.; Woillez, J.; Gravity Collaboration (2020)
    Context. Methods used to detect giant exoplanets can be broadly divided into two categories: indirect and direct. Indirect methods are more sensitive to planets with a small orbital period, whereas direct detection is more ...
  • A dusty veil shading Betelgeuse during its Great Dimming 
    Montargès, M.; Cannon, E.; Lagadec, E.; de Koter, A.; Kervella, P.; Sanchez-Bermudez, J.; Paladini, C.; Cantalloube, F.; Decin, L.; Scicluna, P.; Kravchenko, K.; Dupree, A. K.; Ridgway, S.; Wittkowski, M.; Anugu, N.; Norris, R.; Rau, G.; Perrin, G.; Chiavassa, A.; Kraus, S.; Monnier, J. D.; Millour, F.; Le Bouquin, J. -B; Haubois, X.; Lopez, B.; Stee, P.; Danchi, W. (2021)
    Red supergiants are the most common final evolutionary stage of stars that have initial masses between 8 and 35 times that of the Sun<SUP>1</SUP>. During this stage, which lasts roughly 100,000 years<SUP>1</SUP>, red ...

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