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Spectral classification from the ultraviolet line features of S2/68 spectra. V - Supplement series
The paper presents the ultraviolet classification of more than 450 B-Aand F spectra obtained with the sky survey telescope mounted on the TD1satellite. Concerning abnormal objects, attention is given to the Bestars, the binary stars, the helium weak stars, and the lambda Booobjects. With regard to Be stars, it is concluded that the 1930 Awavelength feature is linked to the existence of either shell structuresor Fe II emission lines in the visual spectral range. In addition, it issuggested that stellar spectra at wavelengths of 1410, 1610-20 and 2400A are equivalent to the He-weak group in the classical range.
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Observation and Astrometry data
| Constellation: | いっかくじゅう座 |
| Right ascension: | 07h00m24.99s |
| Declination: | +01°55'53.5" |
| Apparent magnitude: | 6.745 |
| Distance: | 322.581 parsecs |
| Proper motion RA: | -2.1 |
| Proper motion Dec: | -0.5 |
| B-T magnitude: | 6.587 |
| V-T magnitude: | 6.732 |
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