Other
Scientific paper
Jan 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aj.....95..190p&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 95, Jan. 1988, p. 190-198. Research supported by the University of California and NS
Other
20
Binary Stars, F Stars, Variable Stars, Early Stars, Periodic Variations, Stellar Color, Stellar Spectrophotometry
Scientific paper
Spectrographic observations of VZ CVn and AI Hya are combined with published photometric analyses to establish the properties of the components of these early-F type binaries, both of which show intrinsic photometric variability. The variability of AI Hya has been shown to be probably of the δ Scuti type, so that the determination of its mass and other fundamental properties is of special interest. Both components of AI Hya have evolved out of the main-sequence band. The intrinsic variability of VZ CVn is of longer timescale, but its nature has not been established. The components of this short-period system have a unique anomaly in that both are too cool for their masses and radii and fall below the range of known luminosities for stars of their mass.
No associations
LandOfFree
VZ Canum Venaticorum and AI Hydrae, detached F type binaries with variable components 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 VZ Canum Venaticorum and AI Hydrae, detached F type binaries with variable components, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VZ Canum Venaticorum and AI Hydrae, detached F type binaries with variable components will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1044046