Iron whiskers in supernova SN 1987A

Details Iron whiskers in supernova SN 1987A Iron whiskers in supernova SN 1987A

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.225..157w&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 225, no. 1, p. 157-160

Astronomy and Astrophysics

Astrophysics

2

Dust, Emission Spectra, Infrared Spectra, Iron, Stellar Envelopes, Stellar Mass Ejection, Supernova 1987A, Absorptivity, Flux Density, Optical Thickness, Spectrum Analysis, Stellar Models

Scientific paper

The far-infrared flux measurements for supernova SN 1987A are modeled in
terms of length distributions of iron whiskers. The excess emission
detected at lambda is equivalent to 1.3 micrometers can be explained on
the basis of such a model.

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