Photometric and spectroscopic investigation of carbon stars. I - A speculation about the nature of the light and radial velocity variations of UX Dra. II - A comparison of the light and radial velocity changes of Y CVn

Astronomy and Astrophysics – Astronomy

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Carbon Stars, Eclipsing Binary Stars, Light Curve, Radial Velocity, Stellar Spectrophotometry, Velocity Distribution, Absorption Spectra, Astronomical Photography, Astronomical Spectroscopy, Electrophotometers, Molecular Spectra, Stellar Rotation, Swan Bands

Scientific paper

The photoelectric light curves for the carbon star UX Dra were derived in three colours. Their shape suggests the light curve of an eclipsing binary. The period variations of the star are analyzed on the basis of old photographic observations. The radial velocity curve of the star exhibits a minimum preluding the primary light minima by about 0.15 P. The period P is 336 days. The total absorption in the Swan molecular bands in dependence on the light phase of the star is investigated. The period of variability in molecular absorption equals the period of the radial velocity curve. Three possible mechanisms are considered to explain the light, radial velocity and molecular absorption changes of the star: radial pulsations, rotation of a heterogeneous single star, and occultations of two revolving components.

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