The quadruple system HR 3337

Details The quadruple system HR 3337 The quadruple system HR 3337

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jrasc..79..119b&link_type=abstract

Journal of the Royal Astronomical Society of Canada (ISSN 0035-872X), vol. 79, June 1985, p. 119-129. NSERC-supported research.

Astronomy and Astrophysics

Astronomy

3

Companion Stars, Eclipsing Binary Stars, Light Curve, Orbital Elements, Stellar Orbits, Stellar Spectra, Radial Velocity, Stellar Spectrophotometry

Scientific paper

From spectrograms with a dispersion of 12 Åmm-1 the
orbital elements of both components of this visual-spectroscopic binary
have been derived. The companion having a period of 2.5 days was found
to be an eclipsing binary.

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