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Interstellar reddening in the Southern Hemisphere. I - The UVBY beta observations
The uvby-beta photometric data obtained from a Southern Hemisphereobservational project is presented. A uvby-beta photometric network ofnearly 3900 A and early F stars has been established with the intentthat the stars serve as 'space probes' for measurements of interstellarreddening.
| Walraven photometry of nearby southern OB associations
Homogeneous Walraven (VBLUW) photometry is presented for 5260 stars inthe regions of five nearby southern OB associations: Scorpio Centaurus(Sco OB2), Orion OB1, Canis Major OB1, Monoceros OB1, and Scutum OB2.Derived V and (B - V) in the Johnson system are included.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Corona Australis |
| Ascensió Recta: | 18h51m31.29s |
| Declinació: | -38°51'01.8" |
| Magnitud Aparent: | 8.325 |
| Distancia: | 115.207 parsecs |
| Moviment propi RA: | -1.4 |
| Moviment propi Dec: | -6.2 |
| B-T magnitude: | 8.702 |
| V-T magnitude: | 8.357 |
Catàlegs i designacions:
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