Barry Smalley
Keele University
448 Papers
6.6K Citations
Barry Smalley is an academic researcher from Keele University. The author has contributed to research in topics: Planet & Stars. The author has an hindex of 72, co-authored 443 publications. Previous affiliations of Barry Smalley include University College London & Max Planck Society.
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Papers
Lithium 6104A in Population II stars
A. Ford,R. D. Jeffries,Barry Smalley,Sean G. Ryan,Wako Aoki,Satoshi Kawanomoto,David J. James,John R. Barnes +7 more
TL;DR: In this article, the authors obtained echelle spectroscopy of 14 Population II objects selected from those previously observed by Bonifacio & Molaro (1997) for one object, HD 140283, with S/N exceeding 1000 per 0.018A pixel.
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Discovery of WASP-85Ab: a hot Jupiter in a visual binary system
D. J. A. Brown,David R. Anderson,David J. Armstrong,François Bouchy,A. Collier Cameron,Laetitia Delrez,Amanda P. Doyle,Michaël Gillon,Y. Gómez Maqueo Chew,Leslie Hebb,Guillaume Hébrard,Coel Hellier,Emmanuel Jehin,Monika Lendl,Pierre F. L. Maxted,James McCormac,M. Neveu-VanMalle,Don Pollacco,Didier Queloz,Damien Ségransan,Barry Smalley,Oliver Turner,Amaury H. M. J. Triaud,Stéphane Udry +23 more
TL;DR: In this paper, a transiting hot Jupiter exoplanet WASP-85Ab was discovered, which has a mass of 1.09+/-0.03 M_Jup and a radius of 2.66 days, and has a period of 14.64 days.
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The discovery of rapid oscillations in the magnetic Ap stars HD69013 and HD96237
V. G. Elkin,D. W. Kurtz,Hannah L. Worters,Gautier Mathys,Barry Smalley,F. van Wyk,Alexis M. S. Smith +6 more
TL;DR: In this paper, the detection of short period variations in the stars HD69013 and HD96237 are reported, which belong to the class of chemically peculiar Ap stars of the main sequence Pulsations were found from analysis of high time resolution spectra obtained with the ESO Very Large Telescope using a cross correlation method for wide spectral bands, from lines belonging to rare earth elements and from the H alpha core Pulsation amplitudes reach more than 200 m/s for some lines in HD69009 with a period of 114 min and about 100m/s in HD96
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T Tauri stars in the SuperWASP and NSVS surveys
TL;DR: In this article, a study of the long-term optical variability of young T Tauri stars using previously unpublished data from the Super Wide Angle Search for Planets (SuperWASP) project is presented.
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WASP-157b, a Transiting Hot Jupiter Observed with K2
T. Močnik,David R. Anderson,Duncan A. Brown,A. Collier Cameron,Laetitia Delrez,Michaël Gillon,Coel Hellier,Emmanuel Jehin,Monika Lendl,Monika Lendl,Pierre F. L. Maxted,M. Neveu-VanMalle,Francesco Pepe,Don Pollacco,Didier Queloz,Damien Ségransan,Barry Smalley,John Southworth,Amaury H. M. J. Triaud,Amaury H. M. J. Triaud,Stéphane Udry,Richard G. West +21 more
TL;DR: In this paper, the authors gratefully acknowledge the financial support from the Science and Technology Facilities Council (STFC), under grants ST/J001384/1, ST/M001040/1 and St/M50354X/1.
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