No CrossRef data available.
Article contents
Hyperfine structure radio lines from hot ISM in elliptical galaxies
Published online by Cambridge University Press: 21 October 2010
Abstract
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 278
- Copyright
- Copyright © International Astronomical Union 2010