The initial-final mass relationship from white dwarfs in common proper motion pairs
S. Catalan, J. Isern, E. Garcia-Berro, I. Ribas, C. Allende Prieto, A., Z. Bonanos

TL;DR
This study uses white dwarfs in common proper motion pairs to refine the initial-final mass relationship, especially in the low-mass domain, revealing significant scatter and suggesting it may not be a single-valued function.
Contribution
First to utilize common proper motion pairs for deriving the initial-final mass relationship, providing new insights and updated data, especially for low-mass white dwarfs.
Findings
Updated white dwarf classifications and masses.
Large scatter in the semi-empirical data.
Implication that the initial-final mass relationship may not be single-valued.
Abstract
The initial-final mass relationship of white dwarfs, which is poorly constrained, is of paramount importance for different aspects in modern astrophysics. From an observational perspective, most of the studies up to now have been done using white dwarfs in open clusters. In order to improve the initial-final mass relationship we explore the possibility of deriving a semi-empirical relation studying white dwarfs in common proper motion pairs. We have acquired long-slit spectra of the white dwarf members of the selected common proper motion pairs, as well as high resolution spectra of their companions. From these observations, a full analysis of the two members of each common proper motion pair has lead to the initial and final masses of the white dwarfs. These observations have allowed us to provide updated information for the white dwarfs, since some of them were misclassified. This…
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