Issue |
A&A
Volume 683, March 2024
|
|
---|---|---|
Article Number | A175 | |
Number of page(s) | 5 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/202347816 | |
Published online | 18 March 2024 |
A horseshoe-shaped ring of diffuse emission detected at 1.4 GHz
Midnapore City College, Kuturia, Bhadutala, Paschim Medinipur, West Bengal 721129, India
e-mail: sabya.pal@gmail.com
Received:
28
August
2023
Accepted:
18
December
2023
We identify a horseshoe-shaped ring (HSR) of diffuse emission in J1407+0453 from the Faint Images of Radio Sky at Twenty-cm (FIRST) survey using the Very Large Array telescope at 1.4 GHz. An optical galaxy, SDSS J140709.01+045302.1, is present near the limb of the HSR of J1407+0453, with a spectroscopic redshift of z = 0.13360. The total extent of the source, including the diffuse emission of J1407+0453, is 65 arcsec (with a physical extent of 160 kpc), whereas the diameter of the HSR is approximately 10 arcsec (25 kpc). The flux density of the HSR is ∼47 mJy at 1400 MHz, whereas the flux densities of the whole diffuse emission of J1407+0453 at 1400 MHz and 150 MHz are 172 mJy and 763 mJy, respectively. We measure the radio luminosity of HSR J1407+0453 as 1.94 × 1024 W Hz−1, with a spectral index, α1501400 = −0.67. The black hole mass of J1407+0453 is 5.8 × 108 M⊙. We compare the HSR of diffuse emission of J1407+0453 with other discovered diffuse circular sources. The possible formation scenarios for J1407+0453 are discussed, so as to understand the nature of the source. We present a spectral index map of source J147+0453 to study the spectral properties of the source.
Key words: galaxies: ISM / galaxies: active / galaxies: clusters: intracluster medium / galaxies: kinematics and dynamics
© The Authors 2024
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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