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20032008
most citedA new standard: Age and distance for the open cluster NGC 6791 from the eclipsing binary member V20

79 citations · 193 across the 6 of their papers we have counts for

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astro-ph200879 cited

A new standard: Age and distance for the open cluster NGC 6791 from the eclipsing binary member V20

F. Grundahl, J. V. Clausen, S. Hardis +1

The detached eclipsing binary V20 in the old, metal--rich open cluster NGC 6791 is studied in order to determine highly accurate masses and radii of its components. This allows the…

astro-ph200860 cited

Absolute dimensions of eclipsing binaries. XXVI. Setting a new standard: Masses, radii, and abundances for the F-type systems AD Bootis, VZ Hydrae, and WZ Ophiuchi

J. V. Clausen, G. Torres, H. Bruntt +5

We determine absolute dimensions and abundances for the three F-type main-sequence detached eclipsing binaries AD Boo, VZ Hya, and WZ Oph and perform a detailed comparison with res…

astro-ph200815 cited

Four-colour photometry of eclipsing binaries. XLI uvby light curves for AD Bootis, HW Canis Majoris, SW Canis Majoris, V636 Centauri, VZ Hydrae, and WZ Ophiuchi

J. V. Clausen, L. P. R. Vaz, J. M. Garcia +4

CONTEXT: Accurate mass, radius, and abundance determinations from binaries provide important information on stellar evolution, fundamental to central fields in modern astrophysics…

astro-ph200610 cited

Eclipsing Binaries in Open Clusters

John Southworth

Detached eclipsing binaries are very useful objects for calibrating theoretical stellar models and checking their predictions. Detached eclipsing binaries in open clusters are part…

astro-ph2006

Eclipsing Binary Stars in Open Clusters

John Southworth, J V Clausen

The study of detached eclipsing binaries in open clusters can provide stringent tests of theoretical stellar evolutionary models, which must simultaneously fit the masses, radii, a…

astro-ph200629 cited

Eclipsing binaries observed with the WIRE satellite I. Discovery and photometric analysis of the new bright A0IV eclipsing binary Psi Centauri

H. Bruntt, J. Southworth, G. Torres +3

Determinations of stellar mass and radius with realistic uncertainties at the level of 1% provide important constraints on models of stellar structure and evolution. We present a h…