What is in a radio loud NLS1?

Journal
Date Issued
2018
Author(s)
Antón, S.
•
•
Bizzocchi, L.
•
Afonso, J.
DOI
Abstract
A fraction of Narrow Line Seyfert 1 galaxies (NLS1) are hosted by galaxies that present a disturbed morphology, in some cases hinting for merger processes, that are putative sources of gas replenishment. We have been investigating the poorly studied population of radio loud NLS1 (RL-NLS1) showing a flat radio spectrum, assumed to be the manifestation of the presence of a radio jet. In some of the objects the infrared emission is well fitted by a combination of an AGN component and an "active" host galaxy component like M82, the estimate SFR being in the LIRG/ULIRG range (10-500 Msun/year). In order to better characterize that component, we have been investigating the sub-millimeter/millimeter emission of the sources using APEX. Here we present the results concerning a pilot sample of 2 representative objects.
Coverage
Revisiting Narrow-Line Seyfert 1 Galaxies and their Place in the Universe
Start page
58
Conferenece
Revisiting Narrow-Line Seyfert 1 Galaxies and their Place in the Universe
Conferenece place
Padova
Conferenece date
9-13 April, 2018
Uri
Url
Issn Identifier
1824-8039
Ads BibCode
2018rnls.confE..58A
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

NLS1-2018_058.pdf

Description
Pdf editoriale
Size

343.21 KB

Format

Adobe PDF

Checksum (MD5)

f85fa7a42744f6a87c4564dc04639c20