SIMBAD references

2003A&A...405..227H - Astronomy and Astrophysics, volume 405, 227 (2003/7-1)

The circumstellar structure of the Be shell star φ Persei. II. Modeling.

HUMMEL W. and STEFI S.

Abstract (from CDS):

Erratum to Astron, Astrophys, 2001, 368, 471 (2001A&A...368..471H). We recently modeled the orbital phase variations of the He emission lines of the B2e&sdO shell binary φ Per. The angular velocity law used for that study is found to be not correct. We repeated the whole study using a Keplerian velocity law. The application of a Keplerian velocity has only impact on the emission disk radii which are about 50% larger at 15R* with respect to our previously used velocity law. All other conclusions remain valid.

Abstract Copyright: ∼

Journal keyword(s): line: formation - line: profiles - stars: circumstellar matter - stars: emission-line, Be - stars: binaries: spectroscopic

Simbad objects: 1

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2003A&A...405..227H and select 'bookmark this link' or equivalent in the popup menu