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
Green P
(2019)
A Chandra Study: Are Dwarf Carbon Stars Spun Up and Rejuvenated by Mass Transfer?
in The Astrophysical Journal
Farihi J
(2014)
ALMA and Herschel observations of the prototype dusty and polluted white dwarf G29-38
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
Farihi J
(2016)
Circumstellar debris and pollution at white dwarf stars
in New Astronomy Reviews
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
Ashley R
(2019)
Evidence for bimodal orbital separations of white dwarf-red dwarf binary stars
in Monthly Notices of the Royal Astronomical Society
Farihi J
(2018)
Evidence for halo kinematics among cool carbon-rich dwarfs
in Monthly Notices of the Royal Astronomical Society
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
Gänsicke B
(2016)
HIGH-SPEED PHOTOMETRY OF THE DISINTEGRATING PLANETESIMALS AT WD1145+017: EVIDENCE FOR RAPID DYNAMICAL EVOLUTION
in The Astrophysical Journal Letters
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