activity
20052023
most citedThe Chemical Composition of an Extrasolar Minor Planet

338 citations · 1.1k across the 28 of their papers we have counts for

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Showing 2023Show all

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astro-ph.EP2023

Planetesimals at DZ stars I: chondritic compositions and a massive accretion event

Andrew Swan, Jay Farihi, Carl Melis +4

There is a wealth of evidence to suggest that planetary systems can survive beyond the main sequence. Most commonly, white dwarfs are found to be accreting material from tidally di…

astro-ph.SR20239 cited

An emerging and enigmatic spectral class of isolated DAe white dwarfs

Abbigail K. Elms, Pier-Emmanuel Tremblay, Boris T. Gänsicke +9

Two recently discovered white dwarfs, WDJ041246.84754942.26 and WDJ165335.21100116.33, exhibit H and H Balmer line emission similar to stars in the emerging DAHe class,…

astro-ph.EP2023

TOI-2084 b and TOI-4184 b: two new sub-Neptunes around M dwarf stars

K. Barkaoui, M. Timmermans, A. Soubkiou +67

We present the discovery and validation of two TESS exoplanets orbiting nearby M dwarfs: TOI-2084b, and TOI-4184b. We characterized the host stars by combining spectra from Shane/K…

astro-ph.SR2023

IRAS 00450+7401 and the mid-infrared fade/burst cycle of R Coronae Borealis-type stars

William A. Burris, Carl Melis, Allen W. Shafter +3

We present optical and infrared imaging and spectroscopy of the R Coronae Borealis-type (R Cor Bor) star IRAS 00450+7401. Optical spectra further confirm its classification as a co…

astro-ph.SR2023

New chondritic bodies identified in eight oxygen-bearing white dwarfs

Alexandra E. Doyle, Beth L. Klein, Patrick Dufour +8

We present observations and analyses of eight white dwarf stars that have accreted rocky material from their surrounding planetary systems. The spectra of these helium-atmosphere w…

astro-ph.SR202336 cited

Modest dust settling in the IRAS04302+2247 Class I protoplanetary disk

M. Villenave, L. Podio, G. Duchene +11

We present new VLA observations, between 6.8mm and 66mm, of the edge-on Class~I disk IRAS04302+2247. Observations at 6.8mm and 9.2mm lead to the detection of thermal emission from…