activity
20152024
most citedA Giant Planet Candidate Transiting a White Dwarf

183 citations · 723 across the 14 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR20239 cited

A cool, magnetic white dwarf accreting planetary debris

Stephane Vennes, Adela Kawka, Beth L. Klein +3

We present an analysis of spectroscopic data of the cool, highly magnetic and polluted white dwarf 2MASS J0916-4215. The atmosphere of the white dwarf is dominated by hydrogen, but…

astro-ph.SR202313 cited

Disk or Companion: Characterizing Excess Infrared Flux in Seven White Dwarf Systems with Near-Infrared Spectroscopy

Dylan Owens, Siyi Xu, Elena Manjavacas +7

Excess infrared flux from white dwarf stars is likely to arise from a dusty debris disk or a cool companion. In this work, we present near-infrared spectroscopic observations with…

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.SR2021

Discovery of Beryllium in White Dwarfs Polluted by Planetesimal Accretion

Beth Klein, Alexandra E. Doyle, B. Zuckerman +5

The element beryllium is detected for the first time in white dwarf stars. This discovery in the spectra of two helium-atmosphere white dwarfs was made possible only because of the…

astro-ph.SR2020

Serendipitous Discovery of Nine White Dwarfs With Gaseous Debris Disks

Carl Melis, B. Klein, A. E. Doyle +3

Optical spectroscopic observations of white dwarf stars selected from catalogs based on the Gaia DR2 database reveal nine new gaseous debris disks that orbit single white dwarf sta…

astro-ph.SR202010 cited

Atmospheric Temperature Inversions and He I 5876 Core Profile Structure in White Dwarfs

Beth Klein, Simon Blouin, Diego Romani +7

We report distinctive core profiles in the strongest optical helium line, He I 5876, from high-resolution high-sensitivity observations of spectral type DB white dwarfs. By analyzi…