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
Swan A
(2019)
Most white dwarfs with detectable dust discs show infrared variability
in Monthly Notices of the Royal Astronomical Society: Letters
Wilson D
(2019)
Multiwavelength observations of the EUV variable metal-rich white dwarf GD 394
in Monthly Notices of the Royal Astronomical Society
Dey A
(2019)
Overview of the DESI Legacy Imaging Surveys
in The Astronomical Journal
Hallakoun Na'ama
(2018)
Periodic optical variability and debris accretion in white dwarfs: a test for a causal connection
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
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
Redfield S
(2017)
Spectroscopic Evolution of Disintegrating Planetesimals: Minute to Month Variability in the Circumstellar Gas Associated with WD 1145+017
in The Astrophysical Journal
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
Boyajian T
(2018)
The First Post- Kepler Brightness Dips of KIC 8462852
in The Astrophysical Journal
Rocchetto M
(2015)
The frequency and infrared brightness of circumstellar discs at white dwarfs
in Monthly Notices of the Royal Astronomical Society