Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Triaud, Amaury H.M.J."'
Autor:
Zanazzi, J.J., Triaud, Amaury H.M.J.
Publikováno v:
In Icarus June 2019 325:55-66
Autor:
Sebastian, Daniel, Swayne, Matthew, Maxted, Pierre F.L., Triaud, Amaury H.M.J., Sousa, Sérgio G., Olofsson, Göran, Beck, Mathias, Billot, Nicolas, Hoyer, Sergio, Gill, S., Heidari, N., Martin, David V., Persson, M., Standing, Matthew R., Alibert, Yann, Alonso, Roi, Anglada, Guillem, Asquier, J., Bárczy, Tamás, Barrado, David, Queloz, Didier, et. al.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 519 (3)
Eclipsing binaries are important benchmark objects to test and calibrate stellar structure and evolution models. This is especially true for binaries with a fully convective M-dwarf component for which direct measurements of these stars’ masses and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9702f94fd205d00fc6daffa10bf895d0
https://hdl.handle.net/20.500.11850/615129
https://hdl.handle.net/20.500.11850/615129
Autor:
Seager, Sara, Demory, Brice-Olivier, Bonfils, Xavier, Deming, Drake, Triaud, Amaury H.M.J., Gillon, M.
Publikováno v:
arXiv
Because the planets of a system form in a flattened disk, they are expected to share similar orbital inclinations at the end of their formation. The high-precision photometric monitoring of stars known to host a transiting planet could thus reveal th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________88::2679d5fcfc3f0c4d8a88e4fdfd2512ca
http://hdl.handle.net/1721.1/74054
http://hdl.handle.net/1721.1/74054