The optical spectrum of HD 4004 (WN 4b). Evidence of variability

Authors
Citation
A. Niedzielski, The optical spectrum of HD 4004 (WN 4b). Evidence of variability, ACT ASTRONO, 48(4), 1998, pp. 729-746
Citations number
36
Categorie Soggetti
Space Sciences
Journal title
ACTA ASTRONOMICA
ISSN journal
00015237 → ACNP
Volume
48
Issue
4
Year of publication
1998
Pages
729 - 746
Database
ISI
SICI code
0001-5237(1998)48:4<729:TOSOH4>2.0.ZU;2-P
Abstract
We describe the optical spectrum of Wolf-Rayet star HD 4004 (WN 4b) in the wavelength range from 3900 to 7000 Angstrom. Present observations reveal th e stratification effects in the envelope of this star. Also evidence for va riability of HeII line lambda 5411 is presented. Since no radial velocity v ariations are observed in the optical spectrum of this star we conclude tha t HD 4004 is a single Wolf-Rayet star and the observed emission line profil e changes are of intrinsic nature.