Search Results - "H brard, G."

Theoretical study of the Lyman $\gamma$ line profile of atomic hydrogen perturbed by collisions with protons by Allard, N. F., Kielkopf, J. F., H brard, G., Peek, J. M.

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A transiting giant planet with a temperature between 250K and 430K by Deeg, HJ, Moutou, C, Erikson, A, Csizmadia, Sz, Tingley, B, Barge, P, Bruntt, H, Havel, M, Aigrain, S, Almenara, J M, Alonso, R, Auvergne, M, Baglin, A, Barbieri, M, Benz, W, Bonomo, A S, Borde, P, Bouchy, F, Cabrera, J, Carone, L, Carpano, S, Ciardi, D, Deleuil, M, Dvorak, R, Ferraz-Mello, S, Fridlund, M, Gandolfi, D, Gazzano, J-C, Gillon, M, Gondoin, P, Guenther, E, Guillot, T, Hartog, Rden, Hatzes, A, Hidas, M, Hebrard, G, Jorda, L, Kabath, P, Lammer, H, Leger, A, Lister, T, Llebaria, A, Lovis, C, Mayor, M, Mazeh, T, Ollivier, M, Paetzold, M, Pepe, F, Pont, F, Queloz, D, Rabus, M, Rauer, H, Rouan, D, Samuel, B, Schneider, J, Shporer, A, Stecklum, B, Street, R, Udry, S, Weingrill, J, Wuchterl, G

“…Of the over 400 known exoplanets, there are about 70 planets that transit their central star, a situation that permits the derivation of their basic parameters…”
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