ASCA spectra of EX Hydra Emission lines of Ne, Mg, Si, S, Ar, and Fe have been detected in this ASCA SIS spectrum of the magnetic cataclysmic variable EX Hya. The intensity ratios of these lines prove that X-ray emitting plasma of a range of temperatures (<1 keV to >5 keV) co-exist in this system. Search for an Image: (Enter the name of an object.) Additions or Comments: Have we left anything out? Is there something you would like to have added to this page (a link to your own group's research page, for example...)? IMAGES | By Mission | Stars | Cataclysmic Variables | X-ray Binaries | Pulsars | Supernova Remnants & Planetary Nebulae | Galaxies | Active Galactic Nuclei | Clusters and Groups of Galaxies | X-ray/gamma-ray Background & Deep Fields | Solar System Objects | Gamma Ray Bursts HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public Last modified: Thursday, 26-Jun-2003 13:48:44 EDT