The premaximum spectrum of a Magellanic Cloud nova

Astronomy and Astrophysics – Astronomy

Scientific paper

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Magellanic Clouds, Novae, Stellar Spectra, Variable Stars, H Lines, Stellar Magnitude, Stellar Spectrophotometry

Scientific paper

The premaximum spectrum of a Large Magellanic Cloud nova is described.
The emission-line spectrum appears to correspond to a phase about 5
magnitudes below maximum. The nova showed an unusually rapid decline of
0.5 mag per day at the time of discovery after maximum.

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