Blue outliers
The Largest Blueshifts of [O III] emission line in Two Narrow-Line Quasars
http://arxiv.org/abs/astro-ph/0409546
The Narrow-Line Region of Narrow-Line Seyfert 1 Galaxies
http://arxiv.org/abs/1106.4898
On the nature of Seyfert galaxies with high [OIII]5007 blueshifts
http://arxiv.org/abs/0803.0240
The blueshift of the [O III] emission line in NLS1s
http://arxiv.org/abs/astro-ph/0508570
Searching For the Physical Drivers of Eigenvector 1: Influence of Black Hole Mass and Eddington Ratio
http://arxiv.org/abs/astro-ph/0307367
Kinematic Linkage Between the Broad and Narrow Line Emitting Gas in AGN
http://arxiv.org/abs/astro-ph/0207387
An excess of mid-IR luminous galaxies in Abell 1689?
http://arxiv.org/abs/astro-ph/0007437
There are faraway active galaxies that show a blueshift in their [O III] emission lines. One of the largest blueshifts is found in the narrow-line quasar, PG 1543+489, which has a relative velocity of -1150 km/s.[2] These types of galaxies are called "blue outliers".[2]
http://en.wikipedia.org/wiki/Blueshift
Aoki, Kentaro; Toshihiro Kawaguchi; Kouji Ohta (January 2005). "The Largest Blueshifts of the [O III] Emission Line in Two Narrow-Line Quasars". Astrophysical Journal 618 (2): 601–608. arXiv:astro-ph/0409546. Bibcode:2005ApJ...618..601A. doi:10.1086/426075
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