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The Stars in Camelopardalis OB1: Their Distance and Evolutionary History
An investigation is undertaken of the optically identified Population Iobjects in the Cam OB1 region. From the analysis of these objects it isdetermined that the distance to the Cam OB1 stars is 975+/-90 pc. Atheoretical H-R diagram for the Cam OB1 stars reveals that starformation has been going on in the region for1×106-1×108 yr. At present, the mostactive site of star formation is Cam R1, which shows an asymmetry in thedistribution of optically identified Population I objects. The majorityof the pre-main-sequence stars lie in the northern half of theassociation, while the main-sequence stars and evolved stars lie in thesouthern half.
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Observation and Astrometry data
| Constellation: | きりん座 |
| Right ascension: | 03h20m11.43s |
| Declination: | +62°28'22.5" |
| Apparent magnitude: | 9.321 |
| Proper motion RA: | -4.2 |
| Proper motion Dec: | -1.4 |
| B-T magnitude: | 9.434 |
| V-T magnitude: | 9.331 |
Catalogs and designations:
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