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Submit a new article| 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: | Fourneau |  | 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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