Zobrazeno 1 - 10
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pro vyhledávání: '"De La Reza, R."'
Autor:
de Andrés, F. Llorente, de la Reza, R., Cruz, P., Cuenda-Muñoz, D., Alfaro, E. J., Chavero, C., Cifuentes, C.
This work aims to investigate the behaviour of the lithium abundance in stars with and without detected planets. Our study is based on a sample of 1332 FGK main-sequence stars with measured lithium abundances, for 257 of which planets were detected.
Externí odkaz:
http://arxiv.org/abs/2402.01315
Autor:
de la Reza, R., Chavero, C., Roca-Fàbrega, S., de Andrés, F. Llorente, Cruz, P., Cifuentes, C.
Publikováno v:
A&A 671, A136 (2023)
The nature of the few known solar-mass stars simultaneously containing debris disks and planets remains an open question. A number of works have shown that this property appears to be independent of planetary masses as well as of stellar age, but pos
Externí odkaz:
http://arxiv.org/abs/2302.01850
Publikováno v:
A&A 654, A137 (2021)
We investigate two topics regarding solar mass FGK-type stars, the lithium rotation connection (LRC) and the existence of the "lithium desert". We determine the minimum critical rotation velocity ($v \sin i$) related with the LRC separating slow from
Externí odkaz:
http://arxiv.org/abs/2108.05852
Publikováno v:
Proceedings of the International Astronomical Union, IAU Symposium, Volume 332, pp. 237-241 (2018)
The element boron belongs, together with lithium and beryllium, to a known trio of important elements for the study of evolutionary processes in low mass stars. Because B is the least fragile of this trio to be destroyed in the stellar interiors, it
Externí odkaz:
http://arxiv.org/abs/1911.12856
Autor:
de Oliveira, C. Mendes, Ribeiro, T., Schoenell, W., Kanaan, A., Overzier, R. A., Molino, A., Sampedro, L., Coelho, P., Barbosa, C. E., Cortesi, A., Costa-Duarte, M. V., Herpich, F. R., Hernandez-Jimenez, J. A., Placco, V. M., Xavier, H. S., Abramo, L. R., Saito, R. K., Chies-Santos, A. L., Ederoclite, A., de Oliveira, R. Lopes, Gonçalves, D. R., Akras, S., Almeida, L. A., Almeida-Fernandes, F., Beers, T. C., Bonatto, C., Bonoli, S., Cypriano, E. S., de Lima, Erik V. R., de Souza, R. S., de Souza, G. Fabiano, Ferrari, F., Gonçalves, T. S., Gonzalez, A. H., Gutiérrez-Soto, L. A., Hartmann, E. A., Jaffe, Y., Kerber, L. O., Lima-Dias, C., Lopes, P. A. A., Menendez-Delmestre, K., Nakazono, L. M. I., Novais, P. M., Ortega-Minakata, R. A., Pereira, E. S., Perottoni, H. D., Queiroz, C., Reis, R. R. R., Santos, W. A., Santos-Silva, T., Santucci, R. M., Barbosa, C. L., Siffert, B. B., Sodré Jr., L., Torres-Flores, S., Westera, P., Whitten, D. D., Alcaniz, J. S., Alonso-García, Javier, Alencar, S., Alvarez-Candal, A., Amram, P., Azanha, L., Barbá, R. H., Bernardinelli, P. H., Fernandes, M. Borges, Branco, V., Brito-Silva, D., Buzzo, M. L., Caffer, J., Campillay, A., Cano, Z., Carvano, J. M., Castejon, M., Fernandes, R. Cid, Dantas, M. L. L., Daflon, S., Damke, G., de la Reza, R., de Azevedo, L. J. de Melo, De Paula, D. F., Diem, K. G., Donnerstein, R., Dors, O. L., Dupke, R., Eikenberry, S., Escudero, Carlos G., Faifer, Favio R., Farías, H., Fernandes, B., Fernandes, C., Fontes, S., Galarza, A., Hirata, N. S. T., Katena, L., Gregorio-Hetem, J., Hernández-Fernández, J. D., Izzo, L., Arancibia, M. Jaque, Jatenco-Pereira, V., Jiménez-Teja, Y., Kann, D. A., Krabbe, A. C., Labayru, C., Lazzaro, D., Neto, G. B. Lima, Lopes, Amanda R., Magalhães, R., Makler, M., de Menezes, R., Miralda-Escudé, J., Monteiro-Oliveira, R., Montero-Dorta, A. D., Muñoz-Elgueta, N., Nemmen, R. S., Castellón, J. L. Nilo, Oliveira, A. S., Ortíz, D., Pattaro, E., Pereira, C. B., Quint, B., Riguccini, L., Pinto, H. J. Rocha, Rodrigues, I., Roig, F., Rossi, S., Saha, Kanak, Santos, R., Müller, A. Schnorr, Sesto, Leandro A., Silva, R., Castelli, Analía V. Smith, Teixeira, Ramachrisna, Telles, E., de Souza, R. C. Thom, Thöne, C., Trevisan, M., Postigo, A. de Ugarte, Urrutia-Viscarra, F., Veiga, C. H., Vika, M., Vitorelli, A. Z., Werle, A., Werner, S. V., Zaritsky, D.
The Southern Photometric Local Universe Survey (S-PLUS) is imaging ~9300 deg^2 of the celestial sphere in twelve optical bands using a dedicated 0.8 m robotic telescope, the T80-South, at the Cerro Tololo Inter-American Observatory, Chile. The telesc
Externí odkaz:
http://arxiv.org/abs/1907.01567
Autor:
Chavero, C., de la Reza, R., Ghezzi, L., de Andrés, F. Llorente, Pereira, C. B., Giuppone, C., Pinzón, G.
Dwarf stars with debris discs and planets appear to be excellent laboratories to study the core accretion theory of planets formation. These systems are however, insufficiently studied. In this paper we present the main metallicity and lithium abunda
Externí odkaz:
http://arxiv.org/abs/1905.12066
Autor:
Carone, L., Gandolfi, D., Cabrera, J., Hatzes, A. P., Deeg, H. J., Csizmadia, Sz., Paetzold, M., Weingrill, J., Aigrain, S., Alonso, R., Alapini, A., Almenara, J. -M., Auvergne, M., Baglin, A., Barge, P., Bonomo, A. S., Bordé, P., Bouchy, F., Bruntt, H., Carpano, S., Cochran, W. D., Deleuil, M., Díaz, R. F., Dreizler, S., Dvorak, R., Eisloeffel, J., Eigmueller, P., Endl, M., Erikson, A., Ferraz-Mello, S., Fridlund, M., Gazzano, J. -C., Gibson, N., Gillon, M., Gondoin, P., Grziwa, S., Guenther, E. W., Guillot, T., Hartmann, M., Havel, M., Hébrard, G., Jorda, L., Kabath, P., Léger, A., Llebaria, A., Lammer, H., Lovis, C., MacQueen, P. J., Mayor, M., Mazeh, T., Moutou, C., Nortmann, L., Ofir, A., Ollivier, M., Parviainen, H., Pepe, F., Pont, F., Queloz, D., Rabus, M., Rauer, H., Régulo, C., Renner, S., de la Reza, R., Rouan, D., Santerne, A., Samuel, B., Schneider, J., Shporer, A., Stecklum, B., Tal-Or, L., Tingley, B., Udry, S., Wuchterl, G.
Context: CoRoT is a pioneering space mission whose primary goals are stellar seismology and extrasolar planets search. Its surveys of large stellar fields generate numerous planetary candidates whose lightcurves have transit-like features. An extensi
Externí odkaz:
http://arxiv.org/abs/1110.2384
Autor:
Pasquini, L., Melo, C., Chavero, C., Dravins, D., Ludwig, H. -G., Bonifacio, P., De La Reza, R.
Gravitational redshifts in solar-type main-sequence stars are expected to be some 500 ms$^{-1}$ greater than those in giants. Such a signature is searched for between groups of open-cluster stars which share the same average space motion and thus hav
Externí odkaz:
http://arxiv.org/abs/1011.4635
Publikováno v:
Astrophysical Journal 724 (2010) 154-164
This work presents a homogeneous determination of lithium abundances in a large sample of giant-planet hosting stars (N=117), and a control sample of disk stars without detected planets (N=145). The lithium abundances were derived using a detailed pr
Externí odkaz:
http://arxiv.org/abs/1009.2130
Publikováno v:
Astrophysical Journal 720 (2010) 1290-1302
The metal content of planet hosting stars is an important ingredient which may affect the formation and evolution of planetary systems. Accurate stellar abundances require the determinations of reliable physical parameters, namely the effective tempe
Externí odkaz:
http://arxiv.org/abs/1007.2681