Millimeter Wavelength Lines of Heavy Elements Predicted from the Hot Gas in Supernova Remnants and Galaxy Clusters

Details Millimeter Wavelength Lines of Heavy Elements Predicted from the Hot Gas in Supernova Remnants and Galaxy Clusters Millimeter Wavelength Lines of Heavy Elements Predicted from the Hot Gas in Supernova Remnants and Galaxy Clusters

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sval...10..201s&link_type=gif

Soviet Astronomy Letters, Vol.10, NO.4/JUL-AUG, P. 201, 1984

Astronomy and Astrophysics

Astronomy

21

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