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ASCA Guest Observer Facility

ASCA Science Highlights: Normal Galaxies

Follow the links to images and plots

Normal galaxies contain individual X-ray sources such as supernova remnants and X-ray binaries, and may also contain hot, diffuse gas.
  • As a special example of individual sources, the ASCA mission was lucky to catch the early X-ray emission from SN 1993J in the nearby spiral Galaxy, M81.
  • Diffuse emission from elliptical galaxies such as NGC 4472 indicates the presence of hot gas, gravitationally confined by the presence of dark matter in these ellipticals. The presence of a hard component is also seen with ASCA, which is thought to be due to a collection of X-ray binaries.

This page created by Dr. Koji Mukai (USRA) at the U.S. ASCA Guest Observer Facility.

This file was last modified on Monday, 28-May-2001 18:39:12 EDT
Curator: Michael Arida (SP Sys);
HEASARC Guest Observer Facility

If you have any questions concerning ASCA, visit our Feedback form.

This file was last modified on Monday, 28-May-2001 18:39:12 EDT

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