activity
20122026
most citedThe White Dwarf Binary Pathways Survey IV: Three close white dwarf binaries with G-type secondary stars

42 citations · 112 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

A 500 pc volume-limited sample of hot subluminous stars III. The short-period binary population

H. Dawson, M. Dorsch, J. Munday +16

Hot subdwarf stars of spectral types O and B (sdO/B) in binaries form as products of substantial mass loss near the tip of the red giant branch and offer powerful constraints on bi…

astro-ph.SR2026

An Ultramassive White Dwarf with a Likely Oxygen-Neon Core

Stefan M. Arseneau, J. J. Hermes, Vedant Chandra +4

The core composition of ultramassive white dwarfs remains an open question in stellar evolution. The carbon content of white dwarf cores is critical to their role as progenitors of…

astro-ph.SR2026★ 1 cited

Revisiting the Galactic age-metallicity relation from wide white dwarf-main-sequence binaries

Alberto Rebassa-Mansergas, Iset Tejero-Gómez, Roberto Raddi

The age-metallicity relation (AMR) is a fundamental observational constraint for understanding the chemical evolution of the Galaxy. As reliable cosmochronometers, white dwarfs in…

astro-ph.SR2026★ 1 cited

Constraints on White Dwarf Hydrogen Layer Masses Using Gravitational Redshifts

Stefan M. Arseneau, J. J. Hermes, Maria E. Camisassa +2

The hydrogen envelope is the outermost layer of a DA white dwarf; it makes up the entirety of the stellar photosphere, and yet its typical extent is difficult to model theoreticall…

astro-ph.SR2026★ 7 cited

A 500 pc volume-limited sample of hot subluminous stars II. Atmospheric parameters, mass distribution, and kinematics

H. Dawson, M. Dorsch, S. Geier +30

We present a quantitative spectroscopic and kinematic analysis of a volume-complete sample of hot subluminous stars within 500 pc of the Sun, assembled using accurate parallax meas…

astro-ph.IM2025

Asteroseismology of white dwarfs in the 2040s

Murat Uzundag, Ingrid Pelisoli, Stephane Charpinet +6

White dwarfs, the final evolutionary stage of the vast majority of stars, serve as critical tools for cosmochronology, studies of planetary system evolution, and laboratories for n…

astro-ph.IM2025

The Future of Evolved Planetary Systems

Roberto Raddi, Anna F. Pala, Alberto Rebassa-Mansergas +19

Understanding the formation, evolution, and chemical diversity of exoplanets are now central areas of astrophysics research. White dwarfs provide a uniquely sensitive laboratory fo…

astro-ph.SR2022★ 24 cited

Structure and evolution of ultra-massive white dwarfs in general relativity

L. G. Althaus, M. E. Camisassa, S. Torres +4

We present the first set of constant rest-mass ultra-massive oxygen/neon white dwarf cooling tracks with masses larger than 1.29 Msun which fully take into account the effects of g…

astro-ph.SR2020★ 42 cited

The White Dwarf Binary Pathways Survey IV: Three close white dwarf binaries with G-type secondary stars

M. S. Hernandez, M. R. Schreiber, S. G. Parsons +12

Constraints from surveys of post common envelope binaries (PCEBs) consisting of a white dwarf plus an M-dwarf companion have led to significant progress in our understanding of the…

astro-ph.SR2020★ 21 cited

Mode identification in three pulsating hot subdwarfs observed with TESS satellite

S. K. Sahoo, A. S. Baran, U. Heber +12

We report on the detection of pulsations of three pulsating subdwarf B stars observed by the TESS satellite and our results of mode identification in these stars based on an asympt…

astro-ph.SR2012★ 16 cited

Crossing the Gould Belt in the Orion vicinity

K. Biazzo, J. M. Alcalá, E. Covino +5

We present a study of the large-scale spatial distribution of 6482 RASS X-ray sources in approximately 5000 deg^2 in the direction of Orion. We examine the astrophysical properties…