We present and analyse spectra of the Type IIn supernova (SN) 1994W obtained between 18 and 203 d after explosion. During the luminous phase (first 100 d) the line profiles are composed of three major components: (i) narrow P-Cygni lines with the absorption minima at −700 km s−1; (ii) broad emission...
Research Assistant
AI chat, annotations, notes & similar papers
No comments yet
Be the first to share your thoughts!