Detection of optical coronal emission from 106-K gas in the core of the Centaurus cluster Coronal line emission in NGC 4696 (2011)
Attributed to:
A rolling grant for the observation and study of cosmic X-ray sources (Apr 2009 to Mar 2014)
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2010.17693.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2010.17693.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1