High-resolution mapping of Magellanic Cloud supernova remnants in coronal forbidden Fe XIV

Details High-resolution mapping of Magellanic Cloud supernova remnants in coronal forbidden Fe XIV High-resolution mapping of Magellanic Cloud supernova remnants in coronal forbidden Fe XIV

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...231l.147d&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 231, Aug. 1, 1979, p. L147-L150.

Astronomy and Astrophysics

Astrophysics

24

Forbidden Bands, Magellanic Clouds, Stellar Coronas, Supernova Remnants, X Ray Sources

Scientific paper

Two supernova remnants (N49 and N63 A in the Large Magellanic Cloud) have been mapped in their 5303-A coronal forbidden emission line of Fe XIV at an effective spatial resolution of 2 arcsec. These observations confirm the validity of the cloudlet shock model put forward by McKee and coworkers (1978), and physical parameters are derived for one such cloudlet. Soft X-ray fluxes for these remnants are predicted to be substantially higher than those of the Cygnus Loop.

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