New envelope binding energies derived from PARSEC stellar tracks alter compact binary merger rate densities by over an order of magnitude when used in population synthesis.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.SR 3representative citing papers
Identifies 596 WD-MS binary candidates within 100 pc (497 new) by detecting NUV excess in Gaia sources and fitting SEDs to estimate WD temperatures and masses.
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.
citing papers explorer
-
The impact of envelope binding energies on the merger rate density of binary compact objects
New envelope binding energies derived from PARSEC stellar tracks alter compact binary merger rate densities by over an order of magnitude when used in population synthesis.
-
Revealing Unresolved White Dwarf-Main Sequence Binaries using Gaia DR3 and GALEX I. A Volume limited study of 100 pc
Identifies 596 WD-MS binary candidates within 100 pc (497 new) by detecting NUV excess in Gaia sources and fitting SEDs to estimate WD temperatures and masses.
-
Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.