Abstract
We present imaging and photometric studies of the radio galaxy NGC 1316 (Fornax A) using high spatial resolution near-ultraviolet (NUV) and far-ultraviolet (FUV) imaging telescopes of the first Indian multi-wavelength space observatory AstroSat. The residual maps of UV emission obtained from the subtraction of smooth models witness peculiar features within the central few kpc (1–2 kpc) region. The spatial correspondence between the radio emission maps and FUV imaging study reveal that the UV emitting sources are displaced away from the centre by the AGN outburst (radio jet). The presence of rims and clumpy structures in the outskirt of this galaxy delineate that the galaxy has acquired a large fraction of gas through merger-like events and is still in the process of settling. The estimates of the star formation rates (SFR) using FUV and NUV luminosities are found to be 0.15 \(M_\odot \) yr\(^{-1}\) and 0.36 \(M_\odot \) yr\(^{-1}\), respectively, and provide the lower limit due to the screen effect. The estimated lower rates of SFR in this galaxy probably represent its quenching due to the AGN driven outflows emanating from the central engine of NGC 1316.
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Acknowledgements
We thank the reviewer for encouraging comments and suggestions on the paper. This work uses the data from the AstroSat mission of the Indian Space Research Organisation (ISRO), archived at the Indian Space Science Data Centre (ISSDC). This publication uses UVIT data processed by the payload operations centre at IIA. The UVIT is built in collaboration between IIA, IUCAA, TIFR, ISRO and CSA. Data from VLA and Chandra archive, Extragalactic Database (NED) and NASA’s Astrophysics Data System (ADS) are also used in this paper. NDV thanks Science and Engineering Research Board (SERB), India for providing a research fund (Ref. No.: YSS/2015/001413). NDV also thanks IUCAA, Pune for the use of library facility.
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This article is part of the Special Issue on “AstroSat: Five Years in Orbit”
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Vagshette, N.D., Naik, S., Kumari, N. et al. Imaging and photometric studies of NGC 1316 (Fornax A) using Astrosat/UVIT. J Astrophys Astron 42, 34 (2021). https://doi.org/10.1007/s12036-021-09708-4
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DOI: https://doi.org/10.1007/s12036-021-09708-4