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
Izquierdo P
(2018)
Fast spectrophotometry of WD 1145+017
in Monthly Notices of the Royal Astronomical Society
Koester D
(2014)
The frequency of planetary debris around young white dwarfs
in Astronomy & Astrophysics
Manser CJ
(2019)
A planetesimal orbiting within the debris disc around a white dwarf star.
in Science (New York, N.Y.)
Raddi R
(2015)
Likely detection of water-rich asteroid debris in a metal-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
Rocchetto M
(2015)
The frequency and infrared brightness of circumstellar discs at white dwarfs
in Monthly Notices of the Royal Astronomical Society
Swan A
(2019)
Most white dwarfs with detectable dust discs show infrared variability
in Monthly Notices of the Royal Astronomical Society: Letters
Swan A
(2019)
Interpretation and diversity of exoplanetary material orbiting white dwarfs
in Monthly Notices of the Royal Astronomical Society
Swan A
(2019)
The unbiased frequency of planetary signatures around single and binary white dwarfs using Spitzer and Hubble
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