Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jhu..rept.....c&link_type=abstract
Technical Report, Johns Hopkins Univ. Baltimore, MD United States Space Telescope Science Institute
Astronomy and Astrophysics
Astronomy
Spectral Emission, Spiral Galaxies, Radio Galaxies, Starburst Galaxies, Galactic Radiation, Galaxies, Black Holes (Astronomy), Active Galactic Nuclei, Ultraviolet Emission, Infrared Sources (Astronomy), Ionization
Scientific paper
LINER's (low-ionization nuclear emission-line regions) are found in about 30% of all bright galaxies, including luminous infrared galaxies. They form a heterogeneous class powered by a variety of ionizing mechanisms such as low-luminosity AGNs (active galactic nuclei), starbursts, shocks, or any combination of these. In early-type spirals, LINER's are powered by a low-luminosity AGN, or by an AGN surrounded by circumnuclear star-forming regions. In luminous infrared galaxies, LINER's are powered by starbursts with associated wind-related extended shocks, and an AGN may play a minor role, if any. LINER's in some FR I radio galaxies show strong evidence for the presence of a massive central black hole, and there are indications for the existence of shocks in the nuclear disks of these galaxies. Yet, the dominant ionizing mechanism for LINER's in radio-quiet ellipticals and FR I host galaxies is still unclear. Multifrequency high spatial resolution imaging and spectroscopy are essential to discriminate among the different ionizing mechanisms present in LINER's.
Colina Luis
Koratkar Anuradha
No associations
LandOfFree
The Nature of the Energy Source in LINER's does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Nature of the Energy Source in LINER's, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Nature of the Energy Source in LINER's will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-971977