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N(HI) and Jet Power/Emission in AGNs
Wu, Zhongzu1; Gu, Minfeng2; Zhu, Ming3
AbstractNeutral hydrogen (HI) 21-cm absorption has been detected against very powerful radio jets. In this paper, based on Gupta's sample (Gupta et al. 2006), we present our preliminary study of the correlations between the HI column density N(HI) and the jet power, N(HI) versus the low frequency luminosity at 408 MHz, and N(HI) versus the radio luminosity at 1400 MHz.
KeywordGalaxies: Active Galaxies: Nuclei Quasars: Absorption Lines: Galaxies
Indexed BySCI ; ISTP
WOS IDWOS:000294539300070
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Document Type期刊论文
Affiliation1.Guizhou Univ, Coll Sci, Guiyang 550025, Guizhou, Peoples R China
2.Shanghai Astron Observ, Shanghai 200030, Peoples R China
3.Natl Astron Observ, Beijing 100020, Peoples R China
Recommended Citation
GB/T 7714
Wu, Zhongzu,Gu, Minfeng,Zhu, Ming. N(HI) and Jet Power/Emission in AGNs[J]. JOURNAL OF ASTROPHYSICS AND ASTRONOMY,2011,32(1-2):319-321.
APA Wu, Zhongzu,Gu, Minfeng,&Zhu, Ming.(2011).N(HI) and Jet Power/Emission in AGNs.JOURNAL OF ASTROPHYSICS AND ASTRONOMY,32(1-2),319-321.
MLA Wu, Zhongzu,et al."N(HI) and Jet Power/Emission in AGNs".JOURNAL OF ASTROPHYSICS AND ASTRONOMY 32.1-2(2011):319-321.
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