The radial-velocity variability of Gamma Crucis

Details The radial-velocity variability of Gamma Crucis The radial-velocity variability of Gamma Crucis

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.254...27m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 254, Jan. 1, 1992, p. 27-29.

Astronomy and Astrophysics

Astronomy

8

M Stars, Radial Velocity, Reference Stars, Variable Stars, Astronomical Photometry, Dwarf Stars, Late Stars, Mira Variables, Power Spectra

Scientific paper

High-precision radial velocities of the M3.5III type IAU radial-velocity
standard star Gamma Cru over a period of 2.5 yr have been obtained. The
velocities show that the star is a low-amplitude radial-velocity
variable and is not suitable for use as a precise radial-velocity
standard. The star is probably a variable of the semi-regular class.

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