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Absorption spectra of interstellar grains. I - Reference stars
In order to find the proper standards for the precise extraction ofinterstellar spectral features, an analysis was made of low-resolutionUV spectra of unreddened early-type stars. Stars having a E(B-V) colorexcess below 0.05m contained in the catalog of TD-1 satelliteobservations made during the S2/68 experiment are examined.
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Observation and Astrometry data
| Constellation: | Camelopardalis |
| Right ascension: | 05h42m00.92s |
| Declination: | +76°27'54.2" |
| Apparent magnitude: | 8.209 |
| Distance: | 165.017 parsecs |
| Proper motion RA: | 5.2 |
| Proper motion Dec: | -31.2 |
| B-T magnitude: | 8.304 |
| V-T magnitude: | 8.217 |
Catalogs and designations:
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INHABITED SKY
