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20182025
most cited white dwarfs within 40 pc II: the volume-limited northern hemisphere sample

118 citations · 559 across the 13 of their papers we have counts for

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16 papers · 1 filter

astro-ph.SR2025

MESA Isochrones and Stellar Tracks (MIST) III. The White Dwarf Cooling Sequence

Evan B. Bauer, Aaron Dotter, Charlie Conroy +3

We present a substantial update to the MESA Isochrones and Stellar Tracks (MIST) library, extending the MIST model grids and isochrones down the white dwarf (WD) cooling sequence w…

astro-ph.SR20258 cited

A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr

James Munday, Ruediger Pakmor, Ingrid Pelisoli +9

Double white dwarf binaries are a leading explanation to the origin of type Ia supernovae, but no system exceeding the Chandrasekhar mass limit (1.4 M) has been found that…

astro-ph.SR2025

Comparison of methods used to derive the Galactic star formation history from white dwarf samples

Emily K. Roberts, Pier-Emmanuel Tremblay, Mairi W. O'Brien +4

We compare three methods of deriving the local Galactic star formation history, using as a benchmark the Gaia-defined 40 pc white dwarf sample, currently the largest volume complet…

astro-ph.SR2024

A network of cooler white dwarfs as infrared standards for flux calibration

Abbigail K. Elms, Nicola Pietro Gentile Fusillo, Pier-Emmanuel Tremblay +6

The accurate flux calibration of observational data is vital for astrophysics and cosmology because absolute flux uncertainties of stellar standards propagate into scientific resul…

astro-ph.SR202254 cited

white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere

Mairi W. O'Brien, P. -E. Tremblay, N. P. Gentile Fusillo +31

We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the southern hemisphere. Observations were performed mostly with the Ve…

astro-ph.SR202254 cited

A white dwarf accreting planetary material determined from X-ray observations

Tim Cunningham, Peter J. Wheatley, Pier-Emmanuel Tremblay +4

The atmospheres of a large proportion of white dwarf stars are polluted by heavy elements that are expected to sink out of visible layers on short timescales. This has been interpr…