Comparison of [CII] 158µm line widths to luminosities

A. Samsonyan
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Abstract

Acomparison of [CII] 158µm emission line widths to different luminosities is presented to decide if any luminosity relates to velocity dispersion. [CII] 158 µm emission lines are observed with Herschel PACS for 379 galaxies and the archival data for [CII] line widths are taken from http://cassis.sirtf.com/ herschel/. Emission line widths are compared to [CII] luminosities, to near-infrared 1.6µm luminosities and to infrared 22µm luminosities. H magnitudes are taken from 2MASS catalogue, and 22µm fluxes from the WISE catalogue.
[CII] 158µm线宽与光度的比较
比较了[CII] 158µm发射线宽度对不同光度的影响,以确定光度是否与速度色散有关。[CII]用赫歇尔PACS观测了379个星系的158µm发射线,[CII]线宽的档案数据来自http://cassis.sirtf.com/ Herschel /。发射线宽度与[CII]光度、近红外1.6 μ m光度和红外22 μ m光度进行了比较。H等取自2MASS星表,22µm通量取自WISE星表。
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