1988•The Astronomical JournalRequires access
Spectroscopy of unusual emission-line stars
B. W. Bopp
Open publisher page 4 citations
Abstract
New spectroscopic observations are reported for ten stars that have been identified in the literature as having Hα emission with suspected F, G, or K spectral types. Three of the stars are shown to be Be stars, two are confirmed as early-type supergiants, three show composite (F or K+B) spectra, one is a "post-T Tauri" star, and one is an ordinary F star without emission.