Are All Dwarf Carbon Stars Binary?
Lead Research Organisation:
UNIVERSITY COLLEGE LONDON
Department Name: Physics and Astronomy
Abstract
Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.
Organisations
People |
ORCID iD |
| Jay Farihi (Principal Investigator) |
Publications
Cauley P
(2018)
Evidence for Eccentric, Precessing Gaseous Debris in the Circumstellar Absorption toward WD 1145 + 017
in The Astrophysical Journal Letters
Gänsicke B
(2018)
Broadening of Ly a by neutral helium in DBA white dwarfs
in Monthly Notices of the Royal Astronomical Society
Izquierdo P
(2018)
Fast spectrophotometry of WD 1145+017
in Monthly Notices of the Royal Astronomical Society
Boyajian T
(2018)
The First Post-Kepler Brightness Dips of KIC 8462852
in The Astrophysical Journal Letters
Farihi J
(2018)
Dust production and depletion in evolved planetary systems
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
Wilson T
(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
Wilson D
(2019)
Multiwavelength observations of the EUV variable metal-rich white dwarf GD 394
in Monthly Notices of the Royal Astronomical Society
Green P
(2019)
A Chandra Study: Are Dwarf Carbon Stars Spun Up and Rejuvenated by Mass Transfer?
in The Astrophysical Journal
Dey A
(2019)
Overview of the DESI Legacy Imaging Surveys
in The Astronomical Journal