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pro vyhledávání: '"Calcaferro, L."'
Autor:
Rebassa-Mansergas, A., Solano, E., Jiménez-Esteban, F. M., Torres, S., Rodrigo, C., Ferrer-Burjachs, A., Calcaferro, L. M., Althaus, L. G., Córsico, A. H.
We use the data provided by the Gaia Early Data Release 3 to search for a highly-complete volume-limited sample of unresolved binaries consisting of a white dwarf and a main sequence companion (i.e. WDMS binaries) within 100pc. We select 112 objects
Externí odkaz:
http://arxiv.org/abs/2107.06303
Many low-mass white dwarfs are being discovered in the field of our galaxy and some of them exhibit $g$-mode pulsations, comprising the extremely low-mass variable (ELMV) stars class. Despite it is generally believed that these stars are characterize
Externí odkaz:
http://arxiv.org/abs/1809.09242
Autor:
Córsico, A. H., Althaus, L. G., Calcaferro, L. M., Serenelli, A. M., Kepler, S. O., Jeffery, C. S.
Many extremely low-mass (ELM) white-dwarf (WD) stars are currently being found in the field of the Milky Way. Some of these stars exhibit long-period nonradial $g$-mode pulsations, and constitute the class of ELMV pulsating WDs. In addition, several
Externí odkaz:
http://arxiv.org/abs/1609.01352
Autor:
Fernandez-Lajus, E., Farina, C., Torres, A. F., Schwartz, M. A., Salerno, N., Calderon, J. P., von Essen, C., Calcaferro, L. M., Giudici, F., Llinares, C., Niemela, V.
The periodicity of 5.5 years for some observational events occurring in Eta Carinae manifests itself across a large wavelength range and has been associated with its binary nature. These events are supposed to occur when the binary components are clo
Externí odkaz:
http://arxiv.org/abs/0812.1814
Autor:
Córsico, A. H., Althaus, L. G., Calcaferro, L. M., Serenelli, A. M., Kepler, S. O., Jeffery, C. S.
Publikováno v:
ASP Conference Series; 2017, Vol. 509, p289-294, 6p
Akademický článek
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Autor:
Fern?ndez-Laj?s, E., Fari?a, C., Torres, A., Schwartz, M., Salerno, N., Calder?n, J., von Essen, C., Calcaferro, L., Giudici, F., Llinares, C., Niemela, V.
Publikováno v:
Astronomy and Astrophysics; January 2009, Vol. 493 Issue: 3 p1093-1097, 5p