Evidence for iron whiskers near the galactic centre

Details Evidence for iron whiskers near the galactic centre Evidence for iron whiskers near the galactic centre

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.209..137w&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 209, no. 1, p. 137-141

Astronomy and Astrophysics

Astronomy

2

Carbon, Emission Spectra, Galactic Bulge, Infrared Astronomy, Infrared Spectra, Iron, Line Spectra, Nitrogen, Supernovae, Absorptivity, Abundance, Carbon Monoxide, Far Infrared Radiation

Scientific paper

It is shown that approximately 102 solar mass of iron in the
form of long slender whiskers, expelled from supernovae, can explain an
observed deficit of line emission in the 157.7 micrometer C II line and
in the 205 micrometer N II line from the galactic center region.

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