The Ultraviolet Flare at the Center of the Elliptical Galaxy NGC 4278

Details The Ultraviolet Flare at the Center of the Elliptical Galaxy NGC 4278 The Ultraviolet Flare at the Center of the Elliptical Galaxy NGC 4278

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..199c&link_type=abstract

Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267

Physics

Black Hole Physics, Galaxies: Active, Galaxies: Individual (Ngc 4278), Galaxies: Nuclei, Ultraviolet: Galaxies

Scientific paper

A large fraction of otherwise normal galaxies shows weak nuclear
activity. One of the signatures of the low-luminosity active galactic
nuclei (LLAGNs) is the ultraviolet variability which was serendipitously
discovered in the center of some low-ionization nuclear emission-line
region (LINER) galaxies (see Ho 2008 for a review).

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