J1615+5452: a remnant radio galaxy in the ELAIS-N1 field

Author:

Randriamanakoto Z1,Ishwara-Chandra C H2,Taylor A R345

Affiliation:

1. South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa

2. National Centre for Radio Astrophysics, TIFR, Post Bag No. 3, Ganeshkhind Post, 411007 Pune, India

3. Department of Astronomy, University of Cape Town, Private Bag X3, Rondebosch 7701, South Africa

4. Department of Physics and Astronomy, University of the Western Cape, Private Bag X17, Bellville 7535, South Africa

5. Inter-University Institute for Data Intensive Astronomy, Private Bag X3, Rondebosch 7701, South Africa

Abstract

ABSTRACT We report the discovery of a remnant radio active galactic nucleus (AGN) J1615+5452 in the field of ELAIS-N1. GMRT continuum observations at 150, 325, and 610 MHz combined with archival data from the 1.4 GHz NVSS survey were used to derive the radio spectrum of the source. At a redshift z ∼ 0.33, J1615+5452 has a linear size of ∼100 kpc and spectral indices ranging between $\alpha ^{1400}_{610} \lt -1.5$ and $\alpha ^{325}_{150} = -0.61 \pm 0.12$. While the source has a diffuse radio emission at low frequencies, we do not find evidence of core, jets, or hotspots in the 1.4 GHz VLA data of ∼5 arcsec angular resolution. Such morphological properties coupled with a curved radio spectrum suggest that the AGN fueling mechanisms undergo a shortage of energy supply which is typical of a dying radio AGN. This is consistent with the observed steep curvature in the spectrum Δα ≈ −1, the estimated synchrotron age of $t_{\rm s}=76.0\, ^{+7.4}_{-8.7}$ Myr and a toff/ts ratio of ∼0.3.

Funder

National Research Foundation

Department of Atomic Energy, Government of India

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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