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Sottometti un nuovo articolo| 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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| Costellazione: | Vergine |  | Ascensione retta: | 12h17m57.36s |  | Declinazione: | +11°48'14.7" |  | Magnitudine apparente: | 8.982 |  | Moto proprio RA: | -23.6 |  | Moto proprio Dec: | -11.7 |  | B-T magnitude: | 10.734 |  | V-T magnitude: | 9.127 |  Cataloghi e designazioni:
 
 
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