Hα-wide and narrow-band photometry of R Canis Majoris

H-alpha wide- and narrow-band photoelectric observations of the eclipsing binary R CMa were made at the Biruni Observatory between February 18 and March 2, 1983. The light curves obtained from the observations are analyzed according to Kopal's method for the orbital elements by using frequency-...

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Veröffentlicht in:Astrophysics and space science 1989, Vol.151 (1), p.1-28
Hauptverfasser: EDALATI, M. T, KHALESSE, B, RIAZI, N
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creator EDALATI, M. T
KHALESSE, B
RIAZI, N
description H-alpha wide- and narrow-band photoelectric observations of the eclipsing binary R CMa were made at the Biruni Observatory between February 18 and March 2, 1983. The light curves obtained from the observations are analyzed according to Kopal's method for the orbital elements by using frequency-domain techniques. It appears likely that an exchange has taken place on the angle of the first contact and is probably continuing at the present time. New geometric and photometric elements are derived, and a new value for the angle of the first contact is also given. (Author)
doi_str_mv 10.1007/BF00643626
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source EZB-FREE-00999 freely available EZB journals; SpringerLink Journals - AutoHoldings
subjects Astronomy
Binary and multiple stars
Earth, ocean, space
Eclipsing binaries
Exact sciences and technology
Stars
title Hα-wide and narrow-band photometry of R Canis Majoris
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