Close Binary Systems

By J. Misic. 2009

179 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/ff88f766193eea4541d78420482c95999a056c14

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1. Selma de Mink
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5. M. Prakash
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8. T. Mazeh

Citations in the corpus

• Neutron star observations: Prognosis for equation of state constraints (2006, methodology): “In Newtonian gravity, the Roche radius Rl is well approximated by Kopal’s formula [177] Rl/a = 0.”
• Observational Evidence for Tidal Interaction in Close Binary Systems (2007, methodology): “The parameter k2,1 is the second-order coefficient of the internal structure of the primary, and reflects the stellar radial concentration (e.g., Cowling 1938; Sterne 1939a; b; c; Kopal 1959).”
• Wind Roche-lobe overflow: Application to carbon-enhanced metal-poor stars (2013, methodology): “We choose a minimum value of vw = 5 km s−1, which is consistent with the observations (e.g. Knapp & Morris 1985).”