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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.
| UBV Photoelectric Photometry Catalogue (1986). III Errors and Problems on DM and HD Stars
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| Takýmyýldýz: | Basakci |
| Sað Açýklýk: | 12h44m25.09s |
| Yükselim: | +07°59'50.1" |
| Görünürdeki Parlaklýk: | 8.849 |
| Uzaklýk: | 584.795 parsek |
| özdevim Sað Açýklýk: | -16.9 |
| özdevim Yükselim: | -4.2 |
| B-T magnitude: | 10.809 |
| V-T magnitude: | 9.011 |
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