Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Hans-Jörg Deeg"'
Autor:
Laurance R. Doyle, Hans-Jörg Deeg
Publikováno v:
Symposium - International Astronomical Union. 213:80-84
We investigate the improved detection of extrasolar planets around eclipsing binaries using eclipse minima timing and extrasolar moons around transiting planets using transit timing offered by the upcoming COROT (ESA, 2005), Kepler (NASA, 2007), and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::66c6e3e218f82d4436d95b45c61ecf8e
https://doi.org/10.1017/s0074180900193027
https://doi.org/10.1017/s0074180900193027
Autor:
Sz. Csizmadia, Aviv Ofir, Artie P. Hatzes, S. Carpano, Aldo S. Bonomo, Tsevi Mazeh, Laszlo Szabados, E. W. Guenther, M. Ollivier, Alexandre Santerne, J. M. Almenara, Guillaume Hébrard, Anders Erikson, Pascal Bordé, Davide Gandolfi, Sylvio Ferraz-Mello, Roi Alonso, Rodrigo F. Díaz, Malcolm Fridlund, Hannu Parviainen, J. Schneider, S. Grziwa, P. Klagyivik, Annie Baglin, Martin Pätzold, Juan Cabrera, François Bouchy, Hans-Jörg Deeg, Daniel Rouan, Magali Deleuil, M. Tadeu dos Santos, G. Wuchterl, Heike Rauer, Suzanne Aigrain, Tristan Guillot
Publikováno v:
Astronomy & Astrophysics, 584, A13
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 584, pp.A131. ⟨10.1051/0004-6361/201526763⟩
Astronomy and Astrophysics-A&A, 2015, 584, pp.A131. ⟨10.1051/0004-6361/201526763⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 584, pp.A131. ⟨10.1051/0004-6361/201526763⟩
Astronomy and Astrophysics-A&A, 2015, 584, pp.A131. ⟨10.1051/0004-6361/201526763⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
We report the detection of a rare transiting brown dwarf with a mass of 59 M_Jup and radius of 1.1 R_Jup around the metal-rich, [Fe/H] = +0.44, G9V star CoRoT-33. The orbit is eccentric (e = 0.07) with a period of 5.82 d. The companion, CoRoT-33b, is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::36a55bf9f8c0c02badf9a3fab037eb61
http://hdl.handle.net/1887/48425
http://hdl.handle.net/1887/48425
Publikováno v:
Scientific American. 283:58-65
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::024e460813f2afee23724920add39d16
https://doi.org/10.1038/scientificamerican0900-58
https://doi.org/10.1038/scientificamerican0900-58
Publikováno v:
Acta Astronautica. 46:693-699
The discovery of terrestrial-sized extrasolar planets around main-sequences stars is currently possible from the ground for several sub-solar, small-radii eclipsing binary systems. Terrestrial planets in these systems should form in the binary orbita
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4b251387e96229d33f97c55c05582552
https://doi.org/10.1016/s0094-5765(00)00033-3
https://doi.org/10.1016/s0094-5765(00)00033-3
Publikováno v:
Scopus-Elsevier
For the eclipsing binary system CM Draconis, eclipse minimum times have been monitored with high precision between 1994 and 1999. Periodic deviations of minimum times from a linear ephemeris may indicate the presence of an orbiting third body. Indivi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb5b4c27fb1c14fe794c5ed3752ccbee
Publikováno v:
Proceedings of the International Astronomical Union. 4:406-407
A short overview of the motivation and techniques of the ground-based photometric follow-up program of the CoRoT mission is given.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2d842a367a539a811dc7842694008c5a
https://doi.org/10.1017/s1743921308026781
https://doi.org/10.1017/s1743921308026781
Publikováno v:
Journal of geophysical research. 101(E6)
The detection of terrestrial-sized extrasolar planets from the ground has been thought to be virtually impossible due to atmospheric scintillation limits. However, we show that this is not the case especially selected (but nevertheless main sequence)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a07e0a63ec8ff661928cd95351bf7160
https://pubmed.ncbi.nlm.nih.gov/11539351
https://pubmed.ncbi.nlm.nih.gov/11539351