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.
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Accueil du site > Séminaires > Star Formation in LINER host galaxies
Star Formation in LINER host galaxies at z 0.3
Silvia Tommasin (School of Physics and Astronomy, Tel Aviv University)
Évènements associés
- Le vendredi 11 mai 2012 de 11:00 à 12:00 - lieu : Salle 108, Batiment des Communs - Meudon
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