Titanium oxide radial velocities of long-period variables

Details Titanium oxide radial velocities of long-period variables Titanium oxide radial velocities of long-period variables

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..524d&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, July 1985, p. 524-528) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, July-Aug

Astronomy and Astrophysics

Astronomy

Radial Velocity, Titanium Oxides, Variable Stars, Line Spectra, Masers, Stellar Spectra, Wavelengths

Scientific paper

Radial velocities v(TiO) have been measured for three long-period variables (U Aur, U Ori, R Tau) near maximum light, using the rotational lines of the (C3Delta-X3Delta, 3-0 band in the alpha-system of TiO. Comparison against radial velocities derived from the SiO, H2, OH maser radio lines indicates that the optical velocities v(TiO) similarly appear to represent the motion of the star's center of mass.

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