摘要
An ultraluminous IRAS galaxy sample has been observed at 20cm using the Australia Compact Array (AT). The far infrared luminosity in the sample, log L FIR (L ⊙), is>11 8 ( H 0=50 km s -1 Mpc -1 , q 0=0 5 ). (Radio emission is detected from 19 sources among 37 IRAS galaxies. The radio parameters, for example, peak position, radio flux, etc, are obtained. The radio power P 20cm in the sample is in the range 22 9< log P 20cm (W/Hz) <23 8. The paper presents the preliminary observational results on the sample at 20cm.
An ultraluminous IRAS galaxy sample has been observed at 20cm using the Australia Compact Array (AT). The far infrared luminosity in the sample, log L FIR (L ⊙), is>11 8 ( H 0=50 km s -1 Mpc -1 , q 0=0 5 ). (Radio emission is detected from 19 sources among 37 IRAS galaxies. The radio parameters, for example, peak position, radio flux, etc, are obtained. The radio power P 20cm in the sample is in the range 22 9< log P 20cm (W/Hz) <23 8. The paper presents the preliminary observational results on the sample at 20cm.
出处
《天文研究与技术》
CSCD
1999年第S1期305-308,共4页
Astronomical Research & Technology
