Abstract
Possibilities to detect hostless supernova remnants (hl-SNR) in intergalactic medium using the 1 GHz band of the Square Kilometre Array (SKA) are discussed. The optical detection rate of the hl-SN constrained from the Sloan Digital Sky Survey is used to predict a number of detectable hl-SNRs in the radio band. With an anticipated detection sensitivity (\({\sim }\,1\, \) \(\upmu \)Jy) and angular resolution (\({<}1''\)) with the SKA, a significant number of hl-SNR are expected to get detected in the nearby galaxy groups, such as local group, Virgo, Fornax and Eridanus. A few very luminous hl-SNR may also be detected in the Coma cluster and other rich galaxy clusters up to about 100 Mpc distance. The identification of individual SNRs against other background radio sources will require sub-arcsec angular resolution at 1 GHz to resolve the characteristic circular morphology of the radio SNRs in nearby groups. At larger distances, where individual SNR cannot be resolved, a population of hl-SNR may also be constrained statistically in a small region, by estimating excess unresolved radio sources without a known optical host in a group or cluster, compared to the number density of the background radio sources at \(\upmu \)Jy flux level.
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References
Bhattacharya D. 1990, JApA, 11, 125
Braun R., Bonaldi A., Bourke T., Keane E., Wagg J. 2019, arxiv:1912.12699
Dilday B., et al. 2010, ApJ, 715, 1021
Domainko W., Gitti M., Schindler S., Kapferer W. 2004, A &A, 425, L21
Friedmann M., Maoz D. 2018, MNRAS, 479, 3563
Friemann J. A., et al. 2008, AJ, 135, 338
Gal-Yam A., Maoz D., Guhathakurta P., Filippenko A. V. 2003, AJ, 125, 1087
Graham M. L., Sand D. J., Zaritsky D., Pritchet C. J. 2015, ApJ, 807, 83
Green D. 2004, Bull. Astron. Soc. India, 32, 335
Higdon J., Lingenfelter R. E. 1980, ApJ, 239, 867
Hoeft M., Bruggen M. 2007, MNRAS, 375, 77
Krick J. E., Bernstein R. A. 2007, ApJ, 134, 466
Maoz D., Mannucci F., Brandt T. D. 2012, MNRAS, 426, 3282
Maoz D., Waxman E., Loeb A. 2005, ApJ, 632, 847
McGee S. L., Balogh M. L. 2010, MNRAS, 403, 79
Norris R. P., et al. 2015, in Proceedings of Science, AASKA14, 86, arxiv:1412.6076
Norris R. P., et al. 2021a, PASA, 38, 3
Norris R. P., et al. 2021b, PASA, 38, e046
Omar A. 2019, MNRAS, 484, L141
Omar A. 2022, MNRAS Lett. (in press)
Omar A., Dwarakanath K. S., 2005, JApA, 26, 71
Pavlovic M. Z., Uroševic D., Arbutina B., et al. 2018, ApJ, 852, 84
Reynolds S. P. 2017, Dynamical Evolution and Radiative Processes of Supernova Remnants, in eds Alsabti A., Murdin P., Handbook of Supernovae (Cham: Springer)
Sand D. J., et al. 2011, ApJ, 729, 142
Sand D. J., Zaritsky D., Herbert-Fort S., Sivanandam S., Clowe D. 2008, AJ, 135, 1917
Tang S., Wang Q. D. 2005, ApJ, 628, 205
Tomisaka K., Habe A., Ikeuchi S. 1980, Progress of Theoretical Physics, 64, 1587
Valdarnini R. 2003, MNRAS, 339, 1117
Zaritsky D., Gonzalez A. H., Zabludoff A. I. 2004, ApJ, 613, L93
Zibetti S., White S. D. M., Schneider D. P., Brinkmann J. 2005, MNRAS, 358, 949
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We thank the referee for a critical reading of the manuscript and providing several useful suggestions.
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This article is part of the Special Issue on “Indian Participation in the SKA”.
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Omar, A. Detection possibilities of hostless intergalactic supernova remnants with Square Kilometre Array. J Astrophys Astron 44, 15 (2023). https://doi.org/10.1007/s12036-023-09912-4
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DOI: https://doi.org/10.1007/s12036-023-09912-4