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
Gentile Fusillo N
(2017)
Trace hydrogen in helium atmosphere white dwarfs as a possible signature of water accretion
in Monthly Notices of the Royal Astronomical Society
Bonsor A
(2017)
Infrared observations of white dwarfs and the implications for the accretion of dusty planetary material
in Monthly Notices of the Royal Astronomical Society
Farihi J
(2016)
Circumstellar debris and pollution at white dwarf stars
in New Astronomy Reviews
Wilson D
(2016)
Carbon to oxygen ratios in extrasolar planetesimals
in Monthly Notices of the Royal Astronomical Society
Farihi J
(2016)
Solar abundances of rock-forming elements, extreme oxygen and hydrogen in a young polluted white dwarf
in Monthly Notices of the Royal Astronomical Society
Gänsicke B
(2016)
HIGH-SPEED PHOTOMETRY OF THE DISINTEGRATING PLANETESIMALS AT WD1145+017: EVIDENCE FOR RAPID DYNAMICAL EVOLUTION
in The Astrophysical Journal Letters
Rocchetto M
(2015)
The frequency and infrared brightness of circumstellar discs at white dwarfs
in Monthly Notices of the Royal Astronomical Society
Raddi R
(2015)
Likely detection of water-rich asteroid debris in a metal-polluted white dwarf
in Monthly Notices of the Royal Astronomical Society
Bergfors C
(2014)
Signs of a faint disc population at polluted white dwarfs
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