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Registro de acceso cerrado Stellar physics with the ALHAMBRA photometric system

Autor :Aparicio Villegas, Teresa
Alfaro, Emilio J.
Cabrera-Caño, Jesús
Molés, Mariano
Benítez, Narciso
Perea, Jaime
Olmo, Ascensión del
Fernández-Soto, Alberto
Cristóbal-Hornillos, David
Castander, Francisco J.
Cepa, Jordi
Cerviño, Miguel
González Delgado, Rosa M.
Márquez, I.
Masegosa, J.
Martínez, Vicente J.
Prada, F.
Quintana, José María
Sánchez, Sebastián F.
Fecha de publicación :2011
Editor:Institute of Physics Publishing
Citación :Journal of Physics: Conference Series 328: 012004 (2011)
Resumen:The ALHAMBRA photometric system was specifically designed to perform a tomography of the Universe in some selected areas. Although mainly designed for extragalactic purposes, its 20 contiguous, equal-width, medium-band photometric system in the optical wavelength range, shows a great capacity for stellar classification. In this contribution we propose a methodology for stellar classification and physical parameter estimation (T<SUB>eff</SUB>, log g, [Fe/H], and color excess E(B - V)) based on 18 independent reddening-free Q-values from the ALHAMBRA photometry. Based on the theoretical Spectral library BaSeL 2.2, and applied to 288 stars from the Next Generation spectral Library (NGSL), we discuss the reliability of the method and its dependence on the extinction law used.
URI :http://hdl.handle.net/10261/52133
Identificadores:doi: 10.1088/1742-6596/328/1/012004
issn: 1742-6588
e-issn: 1742-6596
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