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Eight new δ Scuti stars
HD 23194, a member of the Pleiades, was found to pulsate with a periodof about 30min. The literature on the star is reviewed, and it isconcluded that it may be a marginal Am star in a binary system. HD 95321is an evolved Am (ρ Puppis) star with a 5.1-h periodicity. Modeidentification of its pulsation, based on multicolour photometry,suggests that the oscillation is probably non-radial with l=2. We alsoreport on the discovery of six other new δ Scuti stars, some ofwhich may be pulsating in gravity modes.
| Southern metal-poor stars - UBVRI photometry
Considering the study of subdwarf kinematics and metallicities by Eggen,Lynden-Bell, and Sandage (1962), UBVRI photometry and normalizedultraviolet excesses are presented for 178 metal-poor stars, 144 ofwhich are contained in the kinematically unbiased list of Bidelman andMacConnell (1973). The Lowell 0.6 m telescope at Cerro Tololo was used,equipped with a single-channel photometer and a Ga-As photomultiplier.The final magnitudes and colors, number of observations, value ofdelta(U-B)0.6 (if B-V lies between 0.35 and 0.90), B and M class, andpublished spectral types for these stars are presented; severalextremely metal-poor stars are evident. In addition, sixteen nearbyvisual companions of the stars were measured, and their magnitudes andcolors are given.
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Observation and Astrometry data
| Constellation: | ケンタウルス座 |
| Right ascension: | 14h27m18.36s |
| Declination: | -60°58'25.7" |
| Apparent magnitude: | 9.647 |
| Proper motion RA: | -3.1 |
| Proper motion Dec: | -8.3 |
| B-T magnitude: | 10.218 |
| V-T magnitude: | 9.695 |
Catalogs and designations:
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