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The classification of intrinsic variables. VIII - Ultrashort period Cepheids
The photometric and astrometric data for ultrashort-period Cepheids withmaximum visual magnitudes brighter than 11.5 are collected anddiscussed. Most of these variables are high-mass, little-evolved starswhich, in the halo and disk populations, are blue stragglers. Theluminosities are calibrated from membership in disk and halo populationgroups; the visual magnitude equals 8(1-/c1/sub c) for disk stars, where(C1)sub c is a reddening- and temperature-free parameter.
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Observation and Astrometry data
| Constellation: | ろ座 |
| Right ascension: | 03h15m17.11s |
| Declination: | -37°02'30.1" |
| Apparent magnitude: | 8.647 |
| Distance: | 94.787 parsecs |
| Proper motion RA: | 37.7 |
| Proper motion Dec: | -4.8 |
| B-T magnitude: | 9.222 |
| V-T magnitude: | 8.695 |
Catalogs and designations:
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