Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-26T01:49:25.028Z Has data issue: false hasContentIssue false
  • English
  • Français

A wide and collimated radio jet in 3C 84

Published online by Cambridge University Press:  07 April 2020

Gabriele Giovannini
Gabriele Giovannini*
Affiliation:
Physics and Astronomy Dpt, Bologna University, via Gobetti 93/2, 40129 Bologna, Italy Radio Astronomy Institute-INAF, via Gobetti 101 40129, Bologna, Italy email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

I report observations of 3C84 (NGC 1275), the central galaxy of the Perseus cluster, made with an interferometric array including the orbiting radio telescope of the RadioAstron mission. The data transversely resolve the edge-brightened jet in 3C84 only 0.03 mas from the core, which is ten times closer to the central engine than was possible in previous ground-based observations. To better understand physical properties of this peculiar source, I will discuss its present properties in comparison to the past and more recent evolution in the radio band of 3C 84.

Keywords

3C 84VLBI
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S342: Perseus in Sicily: From Black Hole to Cluster Outskirts , May 2018 , pp. 55 - 60
Copyright
© International Astronomical Union 2020

References

Abdo, A. A., et al. 2009, ApJ 699, 31CrossRefGoogle Scholar
Giovannini, G., et al. 2018, Nature Ast., 2, 472CrossRefGoogle Scholar
Kino, M., et al. (2018) 2018, arXiv:180808855Google Scholar
Ko missarov (1990) 1990, Sov. Ast. Lett. 16, 284Google Scholar
Nagai, H., et al. 2012, MNRAS, 423, L122CrossRefGoogle Scholar
Nagai, H., et al. 2014, ApJ, 785, 53CrossRefGoogle Scholar
Nagai, H., et al. 2017, ApJ, 849, 52CrossRefGoogle Scholar
Preuss, E., Kellerman, K. I., Pauliny-Toth, I. I. K., Witzel, A., & Shaffer, D. B. 1979, A&A, 79, 268Google Scholar
Reimer, O., Pohl, M., Sreekumar, P., & Mattox, J. R. 2003, ApJ, 588, 155CrossRefGoogle Scholar
Romney, J. D., Benson, J. M., Dhawan, V., Kellerman, K. I., Vermeulen, R. C., & Walker, R. C. 1995, Proc. Natl. Acad. Sci. USA, 92, 11360CrossRefGoogle Scholar
Suzuki, K., et al. 2012, ApJ, 746, 140CrossRefGoogle Scholar
Venturi, T., Readhead, A. C. S., Marr, J. M., & Backer, D. C. 1993, ApJ, 411, 552CrossRefGoogle Scholar
Walker, R. C., Dhawan, V., Romney, J. D., Kellerman, K. I., & Vermeulen, R. C. 2000, ApJ, 530, 233CrossRefGoogle Scholar