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Three Hot Jupiters transiting K-dwarfs with a significant heavy element mass

Fuente: arXiv

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Bibliographic Details
Main Authors:	Frensch, Y. G. C., Bouchy, F., Curto, G. Lo, Ulmer-Moll, S., Sousa, S. G., Santos, N. C., Stassun, K. G., Watkins, C. N., Chakraborty, H., Barkaoui, K., Battley, M., Ceva, W., Collins, K. A., Daylan, T., Evans, P., Faria, J. P., Jentink, C. Farret, Fontanet, E., Fridén, E., Furesz, G., Gillon, M., Grieves, N., Hellier, C., Jehin, E., Jenkins, J. M., Kwok, L. K. W., Latham, D. W., Lavie, B., Law, N., Mann, A. W., Murgas, F., Palle, E., Parc, L., Pepe, F., Popowicz, A., Pozuelos, F. J., Radford, D. J., Relles, H. M., Revol, A., Ricker, G., Seager, S., Shinde, M., Steiner, M., Strakhov, I. A., Tan, T. -G., Tavella, S., Timmermans, M., Tofflemire, B., Udry, S., Vanderspek, R., Vaulato, V., Winn, J. N., Ziegler, C.
Format:	Preprint
Published:	2025
Subjects:	Earth and Planetary Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2506.04923