We examine new methods of producing and analyzing the empirical initial-final mass relation for open cluster white dwarfs (WDs). We re-determine initial and final masses for the complete sample of published cluster WDs and then pare this sample using stringent criteria. We create an empirical initial-final mass relation by binning all WDs in individual clusters to a single point. Despite potentially significant systematics arising from this approach, we are comfortable concluding that, to within current observational constraints, the initial-final mass relation is linear, any intrinsic scatter in the relation is <~0.05 solar masses, and there is no metallicity dependence. More exploration of these issues is clearly warranted.
Cite
@article{arxiv.astro-ph/0610254,
title = {A New Look at the Empirical Initial-Final Mass Relation},
author = {Kurtis A. Williams},
journal= {arXiv preprint arXiv:astro-ph/0610254},
year = {2007}
}
Comments
6 pages, 2 figures, uses included style file, for publication in the proceedings of the 15th European White Dwarf Workshop. Corrected version fixes a typo that kept a reference from appearing properly