University of Hertfordshire

By the same authors

A Model of the Local WD Population

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Documents

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Original languageEnglish
Title of host publicationIn: Procs of the 14th European Workshop on White Dwarfs - ASP Conference Series 334
PublisherAstronomical Society of the Pacific
Pages93-98
ISBN (Print)1-58381-197-4, 978-1-58381-268-6
Publication statusPublished - 2005

Abstract

We present a model of the solar neighbourhood (d<100 pc) white dwarf (WD) population and show its distribution in e®ective temperature and mass. The WDs are created by the death-rate of a population model matching the local stars observed by hipparcos, considering depletion as caused by the \thin disk" dynamics.

Notes

Original paper can be found at: http://www.astrosociety.org/pubs/cs/328.html--Copyright Astronomical Society of the Pacific

ID: 171973