Are All Dwarf Carbon Stars Binary?
Lead Research Organisation:
UNIVERSITY COLLEGE LONDON
Department Name: Physics and Astronomy
Abstract
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Organisations
People |
ORCID iD |
| Jay Farihi (Principal Investigator) |
Publications
Green P
(2019)
A Chandra Study: Are Dwarf Carbon Stars Spun Up and Rejuvenated by Mass Transfer?
in The Astrophysical Journal
Gänsicke B
(2016)
HIGH-SPEED PHOTOMETRY OF THE DISINTEGRATING PLANETESIMALS AT WD1145+017: EVIDENCE FOR RAPID DYNAMICAL EVOLUTION
in The Astrophysical Journal Letters
Hermes J
(2014)
Heavy metals in a light white dwarf: abundances of the metal-rich, extremely low-mass GALEX J1717+6757
in Monthly Notices of the Royal Astronomical Society
Koester D
(2014)
The frequency of planetary debris around young white dwarfs
in Astronomy & Astrophysics
Raddi R
(2015)
Likely detection of water-rich asteroid debris in a metal-polluted white dwarf
in Monthly Notices of the Royal Astronomical Society
Whitehouse L
(2021)
Carbon-enhanced stars with short orbital and spin periods
in Monthly Notices of the Royal Astronomical Society
Whitehouse L
(2018)
Dwarf carbon stars are likely metal-poor binaries and unlikely hosts to carbon planets
in Monthly Notices of the Royal Astronomical Society
Wyatt M
(2014)
Stochastic accretion of planetesimals on to white dwarfs: constraints on the mass distribution of accreted material from atmospheric pollution
in Monthly Notices of the Royal Astronomical Society
Xu ? S
(2018)
Infrared Variability of Two Dusty White Dwarfs
in The Astrophysical Journal