Diese Anwendung erfordert Java-Skript.

Bitte aktivieren Sie Java-Script in den Browser-Einstellungen.
17th European White Dwarf Workshop: A comprehensive spectroscopic analysis of DB white dwarfs
Bergeron, Pierre (2010)
clipboard
mla
clipboard
Bergeron P. "17th European White Dwarf Workshop: A comprehensive spectroscopic analysis of DB white dwarfs.", timms video, Universität Tübingen (2010): https://timms.uni-tuebingen.de:443/tp/UT_20100816_004_eurowd_0001. Accessed 30 Oct 2020.
apa
clipboard
Bergeron, P. (2010). 17th European White Dwarf Workshop: A comprehensive spectroscopic analysis of DB white dwarfs. timms video: Universität Tübingen. Retrieved October 30, 2020 from the World Wide Web https://timms.uni-tuebingen.de:443/tp/UT_20100816_004_eurowd_0001
harvard
clipboard
Bergeron, P. (2010). 17th European White Dwarf Workshop: A comprehensive spectroscopic analysis of DB white dwarfs [Online video]. 16 August. Available at: https://timms.uni-tuebingen.de:443/tp/UT_20100816_004_eurowd_0001 (Accessed: 30 October 2020).
file download bibtex   endnote
Information
title: 17th European White Dwarf Workshop: A comprehensive spectroscopic analysis of DB white dwarfs
alt. title: 17th European White Dwarf Workshop - Luminosity function, mass distribution and populations
creator: Bergeron, Pierre (author)
subjects: Astronomie, Physik, Astrophysik, Workshop, White Dwarf, Spectroscopic analysis, DB White Dwarfs, Pierre Bergeron
description: 17th European White Dwarf Workshop, 16. bis 20. August 2010
abstract: A Comprehensive Spectroscopic Analysis of DB White Dwarfs (P. Bergeron, F. Wesemael, Pierre Dufour) (Département de Physique, Université de Montréal, Montréal, Québec, Canada) We present a comprehensive spectroscopic survey of over 100 bright DB and DBA white dwarfs selected from the McCook and Sion catalog. Atmospheric parameters are derived for each star from a detailed comparaison of high signal-to-noise optical spectra with an updated version of our model atmosphere grid for DB stars. We discuss in particular the influence of the parameterization of the convective efficiency on the adopted atmospheric parameters. The luminosity function for the DB stars in the Palomar-Green survey is also derived and compared with that of the DA stars in the same survey. We discuss various topics related to our analysis, including the mass distribution of DB and DBA stars as a function of effective temperature, the increase of log g values at low temperatures, and the boundaries of the DB instability strip. We also compare our results with those of the SPY project.
publisher: ZDV Universität Tübingen
contributor: ZDV Universität Tübingen (producer)
creation date: 2010-08-16
dc type: image
localtype: video
identifier: UT_20100816_004_eurowd_0001
language: eng
rights: Url: https://timmsstatic.uni-tuebingen.de/jtimms/TimmsDisclaimer.html?637396148540647381