Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994mnras.269..435b&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Vol. 269, NO. 2/JUL15, P. 435, 1994
Astronomy and Astrophysics
Astronomy
Scientific paper
We apply a null technique to measure to a high accuracy the barycentric radial velocity of the G5 II giant P Lep (HR 1829). We use a magneto-optical filter as a spectroscopic bridge to determine the time at which the geocentric velocity of the star passes through zero. From data taken on the 1.9-m reflector at the South African Astronomical Observatory (SAAO) in 1992 and 1993 January, the barycentric radial velocity of P Lep is calculated to be -13.6+0.2 and -13.576+0.040 km s ' respectively. Key words: techniques: radial velocities - stars: individual: P Lep - stars: oscillations.
Bedford David K.
Chaplin William J.
Davies Alan R.
Innis John L.
Isaak George R.
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