Date:
Tue, 24/04/201212:30-13:30
Location:
Star Formation in LINER host galaxies at z~0.3
Low Ionization Nuclear Emission-line Regions (LINERs) are characterized by low ionization AGN optical emission lines from the center of their host galaxies.
Those latter are found to have a surprisingly high FIRs luminosity by observations with Herschel/PACS of a sample of LINERs at z~0.3.
I will discuss possible causes and consequences of FIR properties of LINERs host galaxies, how they affect the star formation rate estimates, and their connections with the AGN emission.
Those latter are found to have a surprisingly high FIRs luminosity by observations with Herschel/PACS of a sample of LINERs at z~0.3.
I will discuss possible causes and consequences of FIR properties of LINERs host galaxies, how they affect the star formation rate estimates, and their connections with the AGN emission.