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Photometric and spectroscopic analysis of high Galactic latitude molecular clouds. I - Distances and extinctions of stars toward 25 selected regions
The paper presents new photoelectric photometry in the UBV, uvby, andH-beta systems for 320 stars at high Galactic latitudes, selected fortheir proximity to the densest portions of a variety of high Galacticlatitude atomic and molecular clouds. Low-resolution digital spectra areemployed to classify 115 of the stars. Several novel techniques aredeveloped for automatic digital spectral classification, and fordereddening Stromgren uvby-beta and Johnson UBV,H-beta photometry. Anempirical determination of the errors in the derived dereddened colors,and techniques for converting between the two photometric systems arepresented on the basis of the analysis of a statistically significantsample of 1480 stars with complete data sets in both photometric systemsand with an accurate MK spectral type. New constraints on the distancesto several clouds are presented.
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Observation and Astrometry data
| Constellation: | Lièvre |
| Right ascension: | 04h56m26.27s |
| Declination: | -15°22'50.7" |
| Apparent magnitude: | 7.652 |
| Distance: | 194.553 parsecs |
| Proper motion RA: | 2.5 |
| Proper motion Dec: | 12.2 |
| B-T magnitude: | 8.001 |
| V-T magnitude: | 7.681 |
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