The young supernova remnants N132D and 1E 0102.2-7219 - Limits on the presence of rapidly moving sulfur

Details The young supernova remnants N132D and 1E 0102.2-7219 - Limits on the presence of rapidly moving sulfur The young supernova remnants N132D and 1E 0102.2-7219 - Limits on the presence of rapidly moving sulfur

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...371..568l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 371, April 20, 1991, p. 568-570.

Astronomy and Astrophysics

Astrophysics

6

Magellanic Clouds, Nebulae, Sulfur, Supernova Remnants, Supernovae, Abundance, Brightness Distribution, Ionization

Scientific paper

A number of young SNR have rapidly moving knots of oxygen-rich material, including N132D in the LMC and 1E 0102.2-7219 in the SMC. A search was conducted for rapidly moving sulfur in these SNR by observing the forbidden S II 6716 A and forbidden S III 9069, 9532 A lines. Null results were obtained at surface brightnesses a small fraction of those detected in forbidden O III.

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