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Hyperfine structure radio lines from hot ISM in elliptical galaxies

Published online by Cambridge University Press:  21 October 2010

Dmitrijs Docenko
Affiliation:
Institute of Astronomy, University of Latvia, Rainis blvd. 19, Riga, LV-1586, Latvia email: dima@latnet.lv
Rashid A. Sunyaev
Affiliation:
Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, Postfach 1317, 85741 Garching, Germany Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow, Russia
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Abstract

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Hyperfine structure (HFS) line of 14N VII ion with rest frequency of ν = 53.04 GHz should be detectable from the interstellar medium in some of the densest and coolest cores of elliptical galaxies at redshifts exceeding 0.15 or so.

Information

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

Docenko, D. & Sunyaev, R. A. 2007a, in: Böhringer, H., Pratt, G. W., Finoguenov, A., & Schuecker, P. (eds.), Heating versus Cooling in Galaxies and Clusters of Galaxies, ESO Astrophysics Symposia (Berlin, Heidelberg: Springer), p. 333CrossRefGoogle Scholar
Docenko, D. & Sunyaev, R. A. 2007b, in: From Planets to Dark Energy: the Modern Radio Universe, Published online at SISSA, Proceedings of Science, p.90Google Scholar
Sunyaev, R. A. & Churazov, E. M. 1984, Soviet Astron. Lett. 10, 201Google Scholar
Sunyaev, R. A. & Docenko, D. O. 2007, Astron. Lett. 33, 67CrossRefGoogle Scholar