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Quasi-160-minute oscillation period of Delta Scuti stars
The resonance power spectrum (or commensurability spectrum) computed for217 Delta Scuti stars indicates that the dominant (most commensurate)period for the total set of oscillation periods of these stars is 162.2+ or - 2.8 min. Within the error limits, this period coincidesapproximately with the 160-min period of global oscillations of the sun.
| Delta Scuti and related stars
An extensive review is given of the current status of our knowledge ofthe stars in the lower instability strip. Current problems areemphasized. Particular attention is given to the following areas: theconfusion concerning naming and the implied astrophysical properties(often erroneous), single and multiple periods, the effect of rotationand metallicism on pulsation, the nature of the so-called dwarfcepheids, and pulsation in Ap stars. Various reports of unusal andstrange effects are also discussed with personal, possibly biasedjudgment on their reality.
| An Investigation of Short-Period Variable Stars. II. The AI Velorum Stars
Abstract image available at:http://adsabs.harvard.edu/abs/1969ApJS...18..195B
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Member of following groups:
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Observation and Astrometry data
| Constellation: | Grue |
| Right ascension: | 23h09m16.62s |
| Declination: | -40°59'28.3" |
| Apparent magnitude: | 8.735 |
| Distance: | 68.074 parsecs |
| Proper motion RA: | 114.6 |
| Proper motion Dec: | 0.1 |
| B-T magnitude: | 9.561 |
| V-T magnitude: | 8.804 |
Catalogs and designations:
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