Thomas G Wilson
Affiliations: | University College London |
Area:
White dwarf debris disks, the water environment at cometsGoogle:
"Thomas Wilson"Mean distance: (not calculated yet)
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Publications
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Sestito F, Martin NF, Starkenburg E, et al. (2020) The Pristine survey - X. A large population of low-metallicity stars permeates the Galactic disc Monthly Notices of the Royal Astronomical Society. 497 |
Swan A, Farihi J, Wilson TG, et al. (2020) The dust never settles: collisional production of gas and dust in evolved planetary systems Monthly Notices of the Royal Astronomical Society. 496: 5233-5242 |
Swan A, Farihi J, Wilson TG. (2019) Most white dwarfs with detectable dust discs show infrared variability Monthly Notices of the Royal Astronomical Society: Letters. 484: L109-L113 |
Aguado DS, Youakim K, Hernández JIG, et al. (2019) The Pristine survey VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates Monthly Notices of the Royal Astronomical Society. 490: 2241-2253 |
Wilson TG, Farihi J, Gänsicke BT, et al. (2019) The unbiased frequency of planetary signatures around single and binary white dwarfs using Spitzer and Hubble Monthly Notices of the Royal Astronomical Society. 487: 133-146 |
Xu S, Su KYL, Rogers LK, et al. (2018) Infrared Variability of Two Dusty White Dwarfs The Astrophysical Journal. 866: 108 |
Farihi J, van Lieshout R, Cauley PW, et al. (2018) Dust production and depletion in evolved planetary systems Monthly Notices of the Royal Astronomical Society. 481: 2601-2611 |
Whitehouse LJ, Farihi J, Green PJ, et al. (2018) Dwarf carbon stars are likely metal-poor binaries and unlikely hosts to carbon planets Monthly Notices of the Royal Astronomical Society. 479: 3873-3878 |
Wilson TG, Rawlings JMC, Swinyard BM. (2017) Herschel/SPIRE observations of water production rates and ortho-to-para ratios in comets Monthly Notices of the Royal Astronomical Society. 466: 1954-1962 |
Chubb K, Hood R, Wilson T, et al. (2017) Discovering New Variable Stars at Key Stage 3. Physics Education. 52: 35011 |