Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28028| Title: | What is in a radio loud NLS1? | Authors: | Antón, S. CACCIANIGA, Alessandro Bizzocchi, L. Afonso, J. |
Issue Date: | 2018 | Journal: | POS PROCEEDINGS OF SCIENCE | Volume: | Revisiting Narrow-Line Seyfert 1 Galaxies and their Place in the Universe | First Page: | 58 | 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. | Conference Name: | Revisiting Narrow-Line Seyfert 1 Galaxies and their Place in the Universe | Conference Place: | Padova | Conference Date: | 9-13 April, 2018 | URI: | http://hdl.handle.net/20.500.12386/28028 | URL: | https://pos.sissa.it/328/058/ https://pos.sissa.it/328/ |
ISSN: | 1824-8039 | DOI: | 10.22323/1.328.0058 | Bibcode ADS: | 2018rnls.confE..58A | Fulltext: | open |
| Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| NLS1-2018_058.pdf | Pdf editoriale | 343.21 kB | Adobe PDF | View/Open |
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