Please use this identifier to cite or link to this item:
logo share SHARE logo core CORE BASE
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE

Radio continuum and X-ray emission from the most extreme far-IR-excess galaxy NGC 1377: An extremely obscured AGN revealed

AuthorsCostagliola, F.; Herrero-Illana, Rubén CSIC ORCID; Lohfink, A.; Pérez-Torres, Miguel A. CSIC ORCID ; Aalto, S.; Muller, S.; Alberdi, Antxón CSIC ORCID
KeywordsGalaxies: jets
Galaxies: starburst
Radio continuum: galaxies
X-rays: galaxies
Galaxies: individual: NGC 1377
Galaxies: active
Issue Date2016
PublisherEDP Sciences
CitationAstronomy and Astrophysics 594: A114 (2016)
AbstractContext. Galaxies which strongly deviate from the radio-far infrared (FIR) correlation are of great importance for studies of galaxy evolution as they may be tracing early, short-lived stages of starbursts and active galactic nuclei (AGNs). The most extreme FIR-excess galaxy NGC 1377 has long been interpreted as a young dusty starburst, but millimeter observations of CO lines revealed a powerful collimated molecular outflow which cannot be explained by star formation alone. Aims. This paper aims to determine the nature of the energy source in the nucleus of NGC 1377 and to study the driving mechanism of the collimated CO outflow. Methods. We present new radio observations of NGC 1377 at 1.5 and 10 GHz obtained with the Jansky Very Large Array (JVLA) and Chandra X-ray observations. The observations are compared to synthetic starburst models to constrain the properties of the central energy source. Results. We obtained the first detection of the cm radio continuum and X-ray emission in NGC 1377. We found that the radio emission is distributed in two components, one on the nucleus and another offset by 4″5 to the south-west. We confirm the extreme FIR-excess of the galaxy, with a q ≃ 4.2, which deviates by more than 7σ from the radio-FIR correlation. Soft X-ray emission is detected on the off-nucleus component. From the radio emission we estimated for a young (<10 Myr) starburst a star formation rate (SFR) of <0.1 M yr. Such a SFR is not sufficient to power the observed IR luminosity and to drive the CO outflow. Conclusions. We found that a young starburst cannot reproduce all the observed properties of the nucleus of NGC 1377. We suggest that the galaxy may be harboring a radio-quiet, obscured AGN of 10M, accreting at near-Eddington rates. We speculate that the off-nucleus component may be tracing an hot-spot in the AGN jet. © 2016 ESO.
Identifiersdoi: 10.1051/0004-6361/201628997
issn: 1432-0746
Appears in Collections:(IAA) Artículos

Files in This Item:
File Description SizeFormat
IAA_2016_aa28997-16.pdf2,51 MBAdobe PDFThumbnail
Show full item record
Review this work


checked on Nov 23, 2021

Google ScholarTM




WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.