Year: 1974
Type: article
Abstract: Recent spectroscopic data, based on plate material gathered at the Cerro Tololo InterAmerican Observatory, confirm the short period (0.61470 day) velocity changes seen in HD 152667 by Walker (1971). The possibility that this P Cygni star is also a Cephei star is discussed. Key words: variable star - radial velocities - short period
DOI: 10.1086/129634
Institution: Dominion Astrophysical Observatory
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W2048443432
