Results 81 to 90 of about 369 (115)
UBV photometry of eclipsing binaries in the LMC
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BN Pegasi - A Semidetached Eclipsing Binary
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The Reflection Effect in Eclipsing Binary Systems.
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A Millisecond Pulsar in an Eclipsing Binary
Nature, 1988We report the discovery of a remarkable pulsar with period 1.6 ms, moving in a nearly circular 9.17 hour orbit around a low mass companion star. At an observing frequency of 430 MHz, the pulsar, PSR 1957+20, is eclipsed once each orbit for about 50 minutes.
A. S. Fruchter +2 more
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The Eclipsing Binary WX Eridani
International Astronomical Union Colloquium, 1979AbstractThe Algol-type eclipsing binary WX Eridani was observed on 21 nights on the 48-inch telescope of the Japal-Rangapur Observatory during 1973-75 in B and V colours. An improved period of P = 0.82327038 days was obtained from the analysis of the times of five primary minima.
M. B. K. Sarma, K. D. Abhyankar
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AB Andromedae – An overcontact eclipsing binary
New Astronomy, 2021Abstract In an effort to resolve the discrepancy between two earlier studies, new radial velocity and photometric data have been obtained and analyzed by Roche modelling for AB Andromedae, an overcontact W-subtype eclipsing binary. The new values for the basic data, m1 = 0.60 (3) Mʘ, m2 = 1.14 (3) Mʘ, R1 = 0.81 (1) Rʘ, R2 = 1.08 (1) Rʘ, L1 = 0.73 (6)
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Publications of the Astronomical Society of the Pacific, 1956
The observations reported here were obtained in the course of a program of searching for eclipsing binaries which may increase our meager knowledge of the fundamental properties of stars not on the main sequence. Of the stars discussed, three (V694 Aquilae, UU Cancri, and GG Cassiopeiae), while of considerable interest, do not appear promising from ...
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The observations reported here were obtained in the course of a program of searching for eclipsing binaries which may increase our meager knowledge of the fundamental properties of stars not on the main sequence. Of the stars discussed, three (V694 Aquilae, UU Cancri, and GG Cassiopeiae), while of considerable interest, do not appear promising from ...
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Nature, 1988
Tentative d'explication schematique de l'evolution des systemes binaires pouvant donner naissance a des pulsars tres ...
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Tentative d'explication schematique de l'evolution des systemes binaires pouvant donner naissance a des pulsars tres ...
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Fundamental Properties of Late-Type Stars in Eclipsing Binaries
Galaxies, 2022D Baroch +2 more
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