The Interacting Late-type Host Galaxy of the Radio-loud Narrow-line Seyfert 1 IRAS 20181-2244

dc.contributor.authorM. Berton
dc.contributor.authorE. Congiu
dc.contributor.authorS. Ciroi
dc.contributor.authorS. Komossa
dc.contributor.authorM. Frezzato
dc.contributor.authorF. Di Mille
dc.contributor.authorS. Antón
dc.contributor.authorR. Antonucci
dc.contributor.authorA. Caccianiga
dc.contributor.authorP. Coppi
dc.contributor.authorE. Järvelä
dc.contributor.authorJ. Kotilainen
dc.contributor.authorA. Lähteenmäki
dc.contributor.authorS. Mathur
dc.contributor.authorS. Chen
dc.contributor.authorV. Cracco
dc.contributor.authorG. La Mura
dc.contributor.authorP. Rafanelli
dc.contributor.organizationfi=Suomen ESO-keskus|en=Finnish Centre for Astronomy with ESO|
dc.contributor.organization-code1.2.246.10.2458963.20.54954054844
dc.contributor.organization-code2609700
dc.converis.publication-id39178625
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/39178625
dc.date.accessioned2025-08-28T02:13:10Z
dc.date.available2025-08-28T02:13:10Z
dc.description.abstractNarrow-line Seyfert 1 galaxies (NLS1s) are a class of active galactic nuclei that are known to be one of the few sources of gamma-rays, which originate in a relativistic beamed jet. Because of their relatively large distance, a poorly investigated aspect of these jetted NLS1s is their environment, and in particular, their host galaxy. In this work, we present the results of a morphological analysis of the host galaxy of the jetted NLS1 IRAS 20181-2244 observed with the 6.5 m Baade Telescope of the Las Campanas Observatory. The GALFIT analysis run on the Ks image, along with additional spectroscopic observations performed with the Nordic Optical Telescope, clearly revealed the presence of an interacting system of two galaxies. The data suggest that this NLS1 is hosted by a late-type galaxy, although the result is not conclusive. This analysis, along with other results in the literature, might suggest that two populations of jetted NLS1 exist. Further morphological studies are needed to confirm or disprove this hypothesis.
dc.identifier.eissn1538-3881
dc.identifier.jour-issn0004-6256
dc.identifier.olddbid208755
dc.identifier.oldhandle10024/191782
dc.identifier.urihttps://www.utupub.fi/handle/11111/58394
dc.identifier.urnURN:NBN:fi-fe2021042822731
dc.language.isoen
dc.okm.affiliatedauthorBerton, Marco
dc.okm.affiliatedauthorKotilainen, Jari
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherIOP PUBLISHING LTD
dc.publisher.countryUnited Statesen_GB
dc.publisher.countryYhdysvallat (USA)fi_FI
dc.publisher.country-codeUS
dc.relation.articlenumber48
dc.relation.doi10.3847/1538-3881/aaf5ca
dc.relation.ispartofjournalThe Astronomical Journal
dc.relation.issue2
dc.relation.volume157
dc.source.identifierhttps://www.utupub.fi/handle/10024/191782
dc.titleThe Interacting Late-type Host Galaxy of the Radio-loud Narrow-line Seyfert 1 IRAS 20181-2244
dc.year.issued2019

Tiedostot

Näytetään 1 - 1 / 1
Ladataan...
Name:
late-type_radio-loud.pdf
Size:
1.25 MB
Format:
Adobe Portable Document Format
Description:
Publisher's PDF