Type I supernova 1974g in NGC 4414

The paper analyzes six image-tube spectrograms of supernova 1974g in NGC 4414, which were obtained at post-maximum phases of +14 and +40 days over the wavelength range from 4500 to 7000 A with a dispersion of 150 A/mm and a resolution of about 5 A. All features normally seen in this wavelength regio...

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Veröffentlicht in:	Astrophysics and space science 1977-05, Vol.48 (2), p.421-435
Hauptverfasser:	Wyckoff, S., Wehinger, P. A.
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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