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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.
| Spectroscopic studies of stars in ORI OB1 /Belt/ MK spectral classifications are presented for 120 B- and A-type stars inthe Belt subgroup of the Ori OB1 association. Combined with otherpublished spectroscopic data, and the assumed absolute magnitudes givenby Schmidt-Kaler (1965) and Lesh (1979), a mean corrected distancemodulus of 8.56 + or - 0.11 is computed for the eastern region, whilefor the remainder of the Belt a modulus of 8.20 + or - 0.05 is derived.Several B9-A2 subgiants and A7-F0 main-sequence stars were observed inthe western and central regions of the Belt. The ages of these starsimply a spread in formation ages for these subgroups from about 1million yr to at least 10 million yr.
| Photometric studies of stars in ORI OB1 /belt/ Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1979AJ.....84.1846G&db_key=AST
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Miembro de los siguientes grupos:
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Datos observacionales y astrométricos
Constelación: | Orión |
Ascensión Recta: | 05h27m57.50s |
Declinación: | -00°57'30.5" |
Magnitud Aparente: | 8.645 |
Distancia: | 166.389 parsecs |
Movimiento Propio en Ascensión Recta: | -5.7 |
Movimiento Propio en Declinación: | 7.2 |
B-T magnitude: | 9.003 |
V-T magnitude: | 8.675 |
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