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Caltech-NRAO Stripe 82 Survey (CNSS) Paper V: AGNs that transitioned toradio-loud state

Wołowska, Aleksandra and Kunert-Bajraszewska, Magdalena and Mooley, Kunal P. and Siemiginowska, Aneta and Kharb, Preeti and Ishwara-Chandra, C. H. and Hallinan, Gregg and Gromadzki, Mariusz and Kozieł-Wierzbowska, Dorota (2021) Caltech-NRAO Stripe 82 Survey (CNSS) Paper V: AGNs that transitioned toradio-loud state. . (Submitted) https://resolver.caltech.edu/CaltechAUTHORS:20210322-070250837

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Abstract

A recent multi-year Caltech-NRAO Stripe 82 Survey (CNSS) revealed a group of objects that appeared as new radio sources after >5--20 years of absence. They are transient phenomena with respect to the Faint Images of the Radio Sky at Twenty Centimeters (FIRST) survey and constitute the first unbiased sample of renewed radio activity. Here we present the follow-up, radio, optical and X-ray study of them. The group consist of 12 sources, both quasars and galaxies with wide redshift (0.04 < z < 1.7) and luminosity (22 < log₁₀ [L_(1.4GHz)/W Hz⁻¹] > 24.5) distribution. Their radio properties in the first phase of activity, namely the convex spectra and compact morphology, allow them all to be classified as gigahertz-peaked spectrum (GPS) sources. We conclude that the spectral changes are a consequence of the evolution of newly-born radio jets. Our observations show that over the next few years of activity the GPS galaxies keep the convex shape of the spectrum, while GPS quasars rapidly transform into flat-spectrum sources, which may result in them not being recognized as young sources. The wide range of bolometric luminosities, black hole masses and jet powers among the transient sources indicates even greater population diversity in the group of young radio objects. We also suggest that small changes of the accretion disc luminosity (accretion rate) may be sufficient to ignite low-power radio activity that evolves on the scale of decades.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/2103.08422arXivDiscussion Paper
ORCID:
AuthorORCID
Kunert-Bajraszewska, Magdalena0000-0002-6741-9856
Mooley, Kunal P.0000-0002-2557-5180
Kharb, Preeti0000-0003-3203-1613
Hallinan, Gregg0000-0002-7083-4049
Gromadzki, Mariusz0000-0002-1650-1518
Additional Information:We are grateful to Anna Wójtowicz and Łukasz Stawarz for the fruitful discussion. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. We thank the staff of the VLBA and VLA for carrying out these observations in their usual efficient manner. This work made use of the Swinburne University of Technology software correlator, developed as part of the Australian Major National Research Facilities Programme and operated under licence. We thank the staff of the GMRT who have made these observations possible. The GMRT is run by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research. PK and ICH acknowledge the support of the Department of Atomic Energy, Government of India, under the project 12-R&D-TFR-5.02-0700. Some of the observations reported in this paper were obtained with the Southern African Large Telescope (SALT) under programme 2019-1-SCI-023 (PI: A. Wołowska). Polish participation in SALT is funded by grant No. MNiSW DIR/WK/2016/07. This project was supported in part by NASA grant GO8- 19081X (Chandra) and by NASA contract NAS8-03060 to the Chandra X-ray Center (AS). MKB and AW acknowledge support from the ’National Science Centre, Poland’ under grant no. 2017/26/E/ST9/00216. KPM is a Jansky Fellow of the National Radio Astronomy Observatory. KPM and GH acknowledge support from the National Science Foundation Grant AST-1911199. MG is supported by the Polish NCN MAESTRO grant 2014/14/A/ST9/00121. Software: CASA (McMullin et al. 2007), AIPS (van Moorsel et al. 1996), IRAF (Tody 1986, 1993), STARLIGHT (Cid Fernandes et al. 2011), CIAO (Fruscione et al. 2006), Sherpa (Freeman et al. 2001).
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
Department of Atomic Energy (India)12-R&D-TFR-5.02-0700
Ministerstwo Nauki i Szkolnictwa Wyższego (MNiSW)DIR/WK/2016/07
NASAGO8-19081X
NASANAS8-03060
National Science Centre (Poland)2017/26/E/ST9/00216
Jansky FellowshipUNSPECIFIED
National Radio Astronomy ObservatoryUNSPECIFIED
NSFAST-1911199
National Science Centre (Poland)2014/14/A/ST9/00121
Subject Keywords:galaxies: active-galaxies, evolution-galaxies, quasars, recurrent-activity
Record Number:CaltechAUTHORS:20210322-070250837
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210322-070250837
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:108497
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:23 Mar 2021 15:48
Last Modified:23 Mar 2021 15:48

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