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Search for associations containing young stars (SACY). I. Sample and searching method
We report results from a high-resolution optical spectroscopic surveyaimed to search for nearby young associations and young stars amongoptical counterparts of ROSAT All-Sky Survey X-ray sources in theSouthern Hemisphere. We selected 1953 late-type (B-V~≥~0.6),potentially young, optical counterparts out of a total of 9574 1RXSsources for follow-up observations. At least one high-resolutionspectrum was obtained for each of 1511 targets. This paper is the firstin a series presenting the results of the SACY survey. Here we describeour sample and our observations. We describe a convergence method in the(UVW) velocity space to find associations. As an example, we discuss thevalidity of this method in the framework of the β Pic Association.
| 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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Miembro de los siguientes grupos:
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Datos observacionales y astrométricos
| Constelación: | Escorpio |
| Ascensión Recta: | 15h48m09.31s |
| Declinación: | -23°22'24.4" |
| Magnitud Aparente: | 9.683 |
| Movimiento Propio en Ascensión Recta: | -24.2 |
| Movimiento Propio en Declinación: | -29.6 |
| B-T magnitude: | 10.626 |
| V-T magnitude: | 9.761 |
Catálogos y designaciones:
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