The structure at the centre of the giant radio galaxy GRS J0844+4627: a compact symmetric object?

Author:

Marecki A1ORCID,Sebastian B2,Ishwara-Chandra C H3

Affiliation:

1. Institute of Astronomy, Nicolaus Copernicus University, Faculty of Physics, Astronomy and Informatics , ul. Grudziądzka 5, PL-87-100 Toruń, Poland

2. Department of Physics and Astronomy, University of Manitoba , Winnipeg, Canada

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

Abstract

ABSTRACT We observed the core region of the giant radio galaxy GRS J0844+4627 with e-MERLIN at 1.52 and 5.07 GHz. These observations revealed that the apparent single feature at the centre of GRS J0844+4627, as seen by GMRT, consists of two components separated by 2.7 kpc in projection. Follow-up observations at 1.66 GHz using the EVN unveiled the complex morphologies of the two components. In particular, the south-western component identified with the SDSS J084408.85+462744.2 galaxy morphologically resembles a compact symmetric object (CSO) with a projected linear size of 115 pc. If the CSO hypothesis turns out to be correct, then the overall radio structure of GRS J0844+4627 is triple–double. Given that CSOs are considered young objects, GRS J0844+4627 would appear as a recently restarted active galaxy.

Funder

STFC

NASA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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