The spectral variations of MWC 314
Abstract
New spectra of MWC314 are presented; they indicate that the V/R emission line flux ratios show signs of varying in an opposite way to the absorption line radial velocities. The latter appear to be due to apparently non-periodic pulsations, perhaps in strange modes.
- Publication:
-
Active OB Stars: Structure, Evolution, Mass Loss, and Critical Limits
- Pub Date:
- July 2011
- DOI:
- 10.1017/S1743921311011021
- Bibcode:
- 2011IAUS..272..422R
- Keywords:
-
- stars: emission-line;
- Be;
- stars: individual (MWC 314)