pith. sign in

arxiv: astro-ph/9706273 · v1 · pith:XFVXKFX4new · submitted 1997-06-27 · 🌌 astro-ph

The Status of Nova Orionis 1667

classification 🌌 astro-ph
keywords componentsnovabinarycandidateclaimedemission-linefoundhibernating
0
0 comments X
read the original abstract

Images taken in 1.3" seeing show that a claimed hibernating nova, Candidate 5 shown in a Sky & Telescope Newswire item, is found to be a visual binary, with a 1.1" separation between components. Spectra reveal the components to be emission-line M0 and K7 stars.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.