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Optical identifications of the IRAS faint sources in the Virgo cluster area.
This paper presents a study on the deep optical identifications of 369IRAS faint sources in a 102 square degree area centered on the Virgocluster. We obtained the positions and magnitudes of candidates fromfour UK Schmidt Telescope IIIa-J direct plates. 89 (24%) are identifiedas stars and 276 (75%) as galaxies. There are 4 (1%) empty fields to theplate limit of B=~22. The infrared-optical database for 193 FSC-onlysources is given. Most of the IRAS galaxy sources are spirals. There are83 IRAS galaxy sources being regarded as the cluster members by Binggeliet al. (1985). In our sample, a correlation between the luminosity ratioL_IR_/L_B_ and the infrared flux ratio F(100μm)/F(60μm) isevident. For the member galaxies, a weak correlation between L_IR_/L_B_and L_IR_ is also found.
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Miembro de los siguientes grupos:
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Datos observacionales y astrométricos
| Constelación: | Virgo |
| Ascensión Recta: | 12h15m41.98s |
| Declinación: | +10°52'03.5" |
| Magnitud Aparente: | 8.413 |
| Distancia: | 202.84 parsecs |
| Movimiento Propio en Ascensión Recta: | -50.1 |
| Movimiento Propio en Declinación: | 5.5 |
| B-T magnitude: | 9.85 |
| V-T magnitude: | 8.532 |
Catálogos y designaciones:
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