Abstract
The Pulkovo Spectrophotometric Data Base is used to determine the expansion velocities and radii of the continuum emission layers of the stars RR SCO and OMICR CET. Dependences of the radii and velocities on the phase of the variability cycle are found which agree with the known values obtained from the layers which emit line radiation.
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Translated from Astrofizika, Vol. 50, No. 4, pp. 557–564 (November 2007).
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Ruban, E.V., Arkharov, A.A., Hagen-Thorn, E.I. et al. Physical parameters of the continuum emission layer of Mira type stars. II. Radii and expansion velocities. Astrophysics 50, 460–466 (2007). https://doi.org/10.1007/s10511-007-0043-5
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DOI: https://doi.org/10.1007/s10511-007-0043-5