HI absorption detected in an untargeted ASKAP-FLASH sample is statistically over-represented towards young, compact (peaked-spectrum) radio AGN, with derived linear sizes below about 2 kpc.
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Why so young? A curious connection between the broadband flux and neutral gas content of AGN
HI absorption detected in an untargeted ASKAP-FLASH sample is statistically over-represented towards young, compact (peaked-spectrum) radio AGN, with derived linear sizes below about 2 kpc.