skip to content
 
ROSAT Guest Observer Facility

Large Magellanic Cloud

LMC Survey Image

Image credit: Max-Planck-Institut für extraterrestrische Physik (MPE)

ROSAT sources in the Large Magellanic Cloud. The new class of super soft X-ray sources and the galactic foreground stars emerge yellow or red. The nearly five million degree interstellar gas in the LMC is manifested by a diffuse green emission. The super soft X-ray sources are thought to be white dwarfs accreting matter from a binary companion star with a rate sufficient to produce steady nuclear burning on the white dwarf surface. In contrast to other accreting X-ray binaries, where gravitational energy powers the X-ray source, nuclear burning is the primary energy source in super soft X-ray sources.

Curator: Michael Arida (SP Sys); arida@milkyway.gsfc.nasa.gov
HEASARC Guest Observer Facility


Please use the Feedback link if you have questions on ROSAT.

This file was last modified on Thursday, 04-Oct-2007 12:10:10 EDT

NASA Astrophysics

  • FAQ/Comments/Feedback
  • Education Resources
  • Download Adobe Acrobat
  • A service of the Astrophysics Science Division (ASD) at NASA/ GSFC

    ROSAT Project Scientist: Dr. Robert Petre

    Responsible NASA Official: Phil Newman

    Privacy Policy and Important Notices.