Supernova 1994I in NGC 5194

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

B. Schmidt, P. Challis, and R. Kirshner, Center for Astrophysics, report: "A spectrogram obtained with the F. L. Whipple Observatory 1.5-m telescope (+ FAST) on Apr. 5 by P. Berland confirms the conclusion by Filippenko et al. (IAUC 5964) that SN 1994I is not a type-II supernova, as had been reported earlier. The spectrum has strong lines at observed wavelengths 745, 611, 569, 492, 478, 434, and 377 nm, and no hydrogen is detected. M. Phillips, Cerro Tololo Interamerican Observatory, has pointed out that this object's spectrum resembles the pre-maximum spectrum of the type-Ic object SN 1983V."

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