Redefining the empirical ZZ Ceti instability strip

• Autor(a) principal: Mukadam, Anjum Shagufta
• Data de Publicação: 2004
• Outros Autores: Winget, Donald Earl, Von Hippel, Theodore A., Montgomery, Michael Houston, Kepler, Souza Oliveira, Costa, Alex Fabiano Murillo da
• Tipo de documento: Artigo
• Idioma: eng
• Título da fonte: Repositório Institucional da UFRGS
• Texto Completo: http://hdl.handle.net/10183/108915
• topic: Hidrogênio; Atmosferas estelares; Pulsacoes estelares; Espectros estelares; Estrelas variaveis; Anãs brancas; Stars: oscillations; Stars: variables: other; White dwarfs

We use the new ZZ Ceti stars (hydrogen-atmosphere white dwarf variables; DAVs) discovered within the Sloan Digital Sky Survey (Mukadam et al. 2004) to redefine the empirical ZZ Ceti instability strip. This is the first time since the discovery of white dwarf variables in 1968 that we have a homogeneous set of spectra acquired using the same instrument on the same telescope, and with consistent data reductions, for a statistically significant sample of ZZ Ceti stars. The homogeneity of the spectra reduces the scatter in the spectroscopic temperatures, and we find a narrow instability strip of width ~950 K, from 10,850 to 11,800 K. We question the purity of the DAV instability strip, as we find several nonvariables within. We present our best fit for the red edge and our constraint for the blue edge of the instability strip, determined using a statistical approach.