Computer Science
Scientific paper
Feb 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977obs....97....1b&link_type=abstract
The Observatory, vol. 97, Feb. 1977, p. 1, 2.
Computer Science
4
Mira Variables, Radial Velocity, Stellar Magnitude, Stellar Rotation, Variable Stars, Absorption Spectra, Binary Stars, Emission Spectra, Stellar Spectra
Scientific paper
Results are reported for measurements of emission-line and absorption-line radial velocities of six Mira variables at seven maxima, which were performed on spectrograms obtained with a dispersion of 18 A/mm in the spectral region from 3800 to 4500 A. The stars include TW Cyg, TY Cyg, RU Her, X Oph, RR Sgr, and U UMi. Comparison of the results for two stars with previously observed absorption-line radial velocities shows that the mean difference between the two data sets is satisfactorily small.
Barnes Th. G.
Fekel Francis C.
No associations
LandOfFree
Radial velocities of six Mira variables does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Radial velocities of six Mira variables, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial velocities of six Mira variables will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-800477