Zobrazeno 1 - 10
of 196
pro vyhledávání: '"Janot-Pacheco E"'
Autor:
Gomes, R. L., Martins, B. L. Canto, Fontinele, D. O., Almeida, L. A., Freire, R. Alves, Brito, A. C., de Amorim, R. G. S. B., Lopes, C. E. Ferreira, Hazarika, D., Janot-Pacheco, E., Leão, I. C., Messias, Y. S., Souza, R. A. A., De Medeiros, J. R.
Publikováno v:
The Astrophysical Journal, Volume 961, Issue 1, id.55, 12 pp. The Astrophysical Journal, Volume 961 (2024)
We report the discovery of three Transiting Exoplanet Survey Satellite Objects of Interest (TOI) with signatures of pulsation, observed in more than one sector. Our main goal is to explore how large is the variety of classical pulsators such as $\del
Externí odkaz:
http://arxiv.org/abs/2402.15935
Autor:
Kervella, P., Borgniet, S., de Souza, A. Domiciano, Mérand, A., Gallenne, A., Rivinius, Th., Lacour, S., Carciofi, A., Faes, D. Moser, Bouquin, J. -B. Le, Taormina, M., Pilecki, B., Berger, J. -Ph., Bendjoya, Ph., Klement, R., Millour, F., Janot-Pacheco, E., Spang, A., Vakili, F.
Publikováno v:
A&A 667, A111 (2022)
Achernar, the closest and brightest classical Be star, presents rotational flattening, gravity darkening, occasional emission lines due to a gaseous disk, and an extended polar wind. It is also a member of a close binary system with an early A-type d
Externí odkaz:
http://arxiv.org/abs/2209.07537
Autor:
Barraza, L. F., Gomes, R. L., Messias, Y. S., Leão, I. C., Almeida, L. A., Janot-Pacheco, E., Brito, A. C., Brito, F. A. C., Santana, J. V., Gonçalves, N. S., Chagas, M. L. das, Teixeira, M. A., De Medeiros, J. R., Martins, B. L. Canto
Publikováno v:
2022, ApJ, 924, 117B
Stellar rotation is a fundamental observable that drives different aspects of stellar and planetary evolution. In this work, we present an unprecedented manifold analysis of 160 B-type stars with light curves collected by the TESS space mission using
Externí odkaz:
http://arxiv.org/abs/2202.01022
Autor:
Andrade, L., Janot-Pacheco, E., Emilio, M., Frémat, Y., Neiner, C., Poretti, E., Mathias, P., Rainer, M., Suárez, J. C., Uytterhoeven, K., Briquet, M., Diago, P. D., Fabregat, J., Gutiérrez-Soto, J.
Publikováno v:
A&A 603, A41 (2017)
We analyzed the star HD 171219, one of the relatively bright Be stars observed in the seismo field of the CoRoT satellite, in order to determine its physical and pulsation characteristics. Classical Be stars are main-sequence objects of mainly B-type
Externí odkaz:
http://arxiv.org/abs/1705.06971
Autor:
Leão, I. C., Pasquini, L., Lopes, C. E. Ferreira, Neves, V., Valcarce, A. A. R., de Oliveira, L. L. A., da Silva, D. Freire, de Freitas, D. B., Martins, B. L. Canto, Janot-Pacheco, E., Baglin, A., De Medeiros, J. R.
Publikováno v:
A&A 582, A85 (2015)
We study the distribution of the photometric rotation period (Prot), which is a direct measurement of the surface rotation at active latitudes, for three subsamples of Sun-like stars: one from CoRoT data and two from Kepler data. We identify the main
Externí odkaz:
http://arxiv.org/abs/1509.01523
Autor:
Lopes, C. E. Ferreira, Neves, V., Leão, I. C., de Freitas, D. B., Martins, B. L. Canto, da Costa, A. D., Paz-Chinchón, F., Chagas, M. L. Das, Baglin, A., Janot-Pacheco, E., De Medeiros, J. R.
Publikováno v:
A&A 583, A122 (2015)
For 6 years the Convection, Rotation, and Planetary Transits (CoRoT) space mission has acquired photometric data from more than one hundred thousand point sources towards and directly opposite from the inner and outer regions of the Galaxy. The high
Externí odkaz:
http://arxiv.org/abs/1508.05358
Autor:
Rauer, H., Catala, C., Aerts, C., Appourchaux, T., Benz, W., Brandeker, A., Christensen-Dalsgaard, J., Deleuil, M., Gizon, L., Goupil, M. -J., Güdel, M., Janot-Pacheco, E., Mas-Hesse, M., Pagano, I., Piotto, G., Pollacco, D., Santos, N. C., Smith, A., -C., J., Suárez, Szabó, R., Udry, S., Adibekyan, V., Alibert, Y., Almenara, J. -M., Amaro-Seoane, P., Eiff, M. Ammler-von, Asplund, M., Antonello, E., Ball, W., Barnes, S., Baudin, F., Belkacem, K., Bergemann, M., Bihain, G., Birch, A. C., Bonfils, X., Boisse, I., Bonomo, A. S., Borsa, F., Brandão, I. M., Brocato, E., Brun, S., Burleigh, M., Burston, R., Cabrera, J., Cassisi, S., Chaplin, W., Charpinet, S., Chiappini, C., Church, R. P., Csizmadia, Sz., Cunha, M., Damasso, M., Davies, M. B., Deeg, H. J., DÍaz, R. F., Dreizler, S., Dreyer, C., Eggenberger, P., Ehrenreich, D., Eigmüller, P., Erikson, A., Farmer, R., Feltzing, S., Fialho, F. de Oliveira, Figueira, P., Forveille, T., Fridlund, M., García, R. A., Giommi, P., Giuffrida, G., Godolt, M., da Silva, J. Gomes, Granzer, T., Grenfell, J. L., Grotsch-Noels, A., Günther, E., Haswell, C. A., Hatzes, A. P., Hébrard, G., Hekker, S., Helled, R., Heng, K., Jenkins, J. M., Johansen, A., Khodachenko, M. L., Kislyakova, K. G., Kley, W., Kolb, U., Krivova, N., Kupka, F., Lammer, H., Lanza, A. F., Lebreton, Y., Magrin, D., Marcos-Arenal, P., Marrese, P. M., Marques, J. P., Martins, J., Mathis, S., Mathur, S., Messina, S., Miglio, A., Montalban, J., Montalto, M., Monteiro, M. J. P. F. G., Moradi, H., Moravveji, E., Mordasini, C., Morel, T., Mortier, A., Nascimbeni, V., Nelson, R. P., Nielsen, M. B., Noack, L., Norton, A. J., Ofir, A., Oshagh, M., Ouazzani, R. -M., Pápics, P., Parro, V. C., Petit, P., Plez, B., Poretti, E., Quirrenbach, A., Ragazzoni, R., Raimondo, G., Rainer, M., Reese, D. R., Redmer, R., Reffert, S., Rojas-Ayala, B., Roxburgh, I. W., Salmon, S., Santerne, A., Schneider, J., Schou, J., Schuh, S., Schunker, H., Silva-Valio, A., Silvotti, R., Skillen, I., Snellen, I., Sohl, F., Sousa, S. G., Sozzetti, A., Stello, D., Strassmeier, K. G., Švanda, M., Szabó, Gy. M., Tkachenko, A., Valencia, D., van Grootel, V., Vauclair, S. D., Ventura, P., Wagner, F. W., Walton, N. A., Weingrill, J., Werner, S. C., Wheatley, P. J., Zwintz, K.
PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it addresses fundamental questions such as: How do planetary systems form
Externí odkaz:
http://arxiv.org/abs/1310.0696
Autor:
De Medeiros, J. R., Lopes, C. E. Ferreira, Leao, I. C., Martins, B. L. Canto, Catelan, M., Baglin, A., Vieira, S., Bravo, J. P., Cortes, C., de Freitas, D. B., Janot-Pacheco, E., Maciel, S. C., Melo, C. H. F., Osorio, Y., de Mello, G. F. Porto, Valio, A.
To date, the CoRoT space mission has produced more than 124,471 light curves. Classifying these curves in terms of unambiguous variability behavior is mandatory for obtaining an unbiased statistical view on their controlling root-causes. The present
Externí odkaz:
http://arxiv.org/abs/1305.0811
Autor:
Emilio, M., Andrade, L., Janot-Pacheco, E., Baglin, A., Gutiérrez-Soto, J., Suárez, J. C., de Batz, B., Diago, P., Fabregat, J., Floquet, M., Frémat, Y., Huat, A. L., Hubert, A. M., Lara, F. Espinosa, Leroy, B., Martayan, C., Neiner, C., Semaan, T., Suso, J.
Classical Be stars are rapid rotators of spectral type late O to early A and luminosity class V-III, wich exhibit Balmer emission lines and often a near infrared excess originating in an equatorially concentrated circumstellar envelope, both produced
Externí odkaz:
http://arxiv.org/abs/1010.5576
Rotationally-split modes can provide valuable information about the internal rotation profile of stars. This has been used for years to infer the internal rotation behavior of the Sun. The present work discusses the potential additional information t
Externí odkaz:
http://arxiv.org/abs/1004.0609