A New Absorption - Line Orbit for the Symbiotic Nova AG Pegasi
Abstract
Precise cross-correlation absorption-line velocities have been derived using high resolution near infrared coudé spectra for the symbiotic nova AG Pegasi. A revised weighted orbital solution is presented based on both extant photographic and the new absorption-line velocities.
- Publication:
-
IAU Colloq. 103: The Symbiotic Phenomenon
- Pub Date:
- 1988
- DOI:
- 10.1007/978-94-009-2969-2_54
- Bibcode:
- 1988ASSL..145..265S