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The region of Collinder 121
The distribution of bright B-type stars in a field with a radius of5° centred at the Galactic open cluster Cr 121 is studied utilizingStrömgren and Hβ photometry. All PPM stars earlier thanspectral type A0 are used, revealing a loose nearby structure at adistance of 660-730pc, and a compact more distant group, which appearsto be a genuine cluster: Cr 121. Based on similar coordinates, distancesand positions on the colour-magnitude (CM) and Hertzsprung-Russell (HR)diagrams, 11 photometric cluster members are selected at a mean distanceof 1085(+/-41 standard error) pc. The results are discussed in the lightof both classical and Hipparcos points of view.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Canis Major |
| Ascensió Recta: | 07h06m50.89s |
| Declinació: | -24°22'48.9" |
| Magnitud Aparent: | 9.887 |
| Moviment propi RA: | 0.8 |
| Moviment propi Dec: | 8.9 |
| B-T magnitude: | 9.945 |
| V-T magnitude: | 9.892 |
Catàlegs i designacions:
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INHABITED SKY
