Supernova 1998bu in M96 - an amateur spectrum

Details Supernova 1998bu in M96 - an amateur spectrum Supernova 1998bu in M96 - an amateur spectrum

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jbaa..108..225g&link_type=abstract

Journal of the British Astronomical Association, vol.108, no.4, p.225

Astronomy and Astrophysics

Astronomy

Scientific paper

Positive proof of a supernova (SN) is found in its distinctive spectrum, and long exposures via a large telescope (>1m aperture) are the norm because of the inherent faintness of the target in the spectroscope. The resultant spectrograms provide a wealth of information for professionals in excess of that required to confirm a SN. However Type Ia SNe at outburst typically show a broad absorption band from 600nm-630nm (Si II) and Type II hydrogen emission lines which place brighter SN within range of a low resolution spectroscope and a modest telescope.

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