77 citations · 228 across the 12 of their papers we have counts for
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astro-ph.SR2018
An Improved Orbital Period for GY Cancri Based on Two K2 Campaigns
Luis Alberto Canizares, Peter Garnavich, Colin Littlefield +4
GY Cnc is a deeply eclipsing cataclysmic variable star with an orbital period of 4.21 hours that has shown several dwarf nova outbursts. The variable was continuously observed by t…
astro-ph.SR2012★ 8 cited
A study of non-Keplerian velocities in observations of spectroscopic binary stars
John B. Hearnshaw, Siramas Komonjinda, Jovan Skuljan +1
This paper presents an orbital analysis of six southern single-lined spectroscopic binary systems. The systems selected were shown to have circular or nearly circular orbits (e < 0…