Journal
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS
Volume 399, Issue 1, Pages 1-70Publisher
ELSEVIER
DOI: 10.1016/j.physrep.2004.07.001
Keywords
white dwarfs; stars : fundamental parameters; stars : kinematics; planetary systems; galaxy : stellar content
Categories
Ask authors/readers for more resources
Old, cool white dwarfs convey valuable information about the early history of our Galaxy. They have been used to determine the age of the Galactic disk, several open clusters and a globular cluster. We review the current understanding of the physics of cool white dwarfs, including their mass distribution, chemical evolution, and cooling. We also examine the role of white dwarfs as tracers of various stellar populations, both in terms of observational searches and theoretical models. (C) 2004 Elsevier B.V. All rights reserved.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available