Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.221..975j&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 221, Aug. 15, 1986, p. 975-991. SERC-supported research
Astronomy and Astrophysics
Astronomy
15
B Stars, Radial Velocity, Variable Stars, Helium, Light Curve, Stellar Gravitation, Tables (Data), Velocity Distribution
Scientific paper
New radial velocity data for the pulsating extreme helium star V652 Her (BD +13°3224) have been obtained with a time resolution of 100 s. High-frequency structure in the radial velocity curve is detected, and a comparison with previous data suggests that the detailed shape of the velocity curve is variable. The data imply that the effective surface gravity must increase by a factor of 4 at minimum radius.
Hill Philip W.
Jeffery Simon C.
No associations
LandOfFree
The pulsating extreme helium star BD+13 deg 3224 (V652 Her). III - The radial velocity curve 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 The pulsating extreme helium star BD+13 deg 3224 (V652 Her). III - The radial velocity curve, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The pulsating extreme helium star BD+13 deg 3224 (V652 Her). III - The radial velocity curve will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-893881