Title:
The angular diameter and distance of the Cepheid ζ Geminorum
Authors:
Kervella, P.; Coudé du Foresto, V.; Perrin, G.; Schöller, M.; Traub, W. A.; Lacasse, M. G.
Affiliation:
AA(European Southern Observatory, Karl-Schwarzschildstr. 2, 85748 Garching, Germany), AB({Observatoire de Paris-Meudon, 5 place Jules Janssen, 92195 Meudon Cedex, France}), AC({Observatoire de Paris-Meudon, 5 place Jules Janssen, 92195 Meudon Cedex, France}), AD(European Southern Observatory, Karl-Schwarzschildstr. 2, 85748 Garching, Germany), AE({Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA}), AF({Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA})
Journal:
Astronomy and Astrophysics, v.367, p.876-883 (2001) (A&A Homepage)
Publication Date:
03/2001
Origin:
A&A
A&A Keywords:
STARS: DISTANCES, STARS: INDIVIDUAL: ZETA GEM, STARS: OSCILLATIONS, STARS: CEPHEIDS, TECHNIQUES: INTERFEROMETRIC
Abstract Copyright:
(c) 2001: Astronomy & Astrophysics
Bibliographic Code:
2001A&A...367..876K

Abstract

Cepheids are the primary distance indicators for extragalactic astronomy and therefore are of very high astrophysical interest. Unfortunately, they are rare stars, situated very far from Earth. Though they are supergiants, their typical angular diameter is only a few milliarcseconds, making them very challenging targets even for long-baseline interferometers. We report observations that were obtained in the K' band (2-2.3 mu m), on the Cepheid zeta Geminorum with the FLUOR beam combiner, installed at the IOTA interferometer. The mean uniform disk angular diameter was measured to be 1.64 +0.14 -0.16 mas. Pulsational variations are not detected at a significant statistical level, but future observations with longer baselines should allow a much better estimation of their amplitude. The distance to zeta Gem is evaluated using Baade-Wesselink diameter determinations, giving a distance of 502 +/- 88 pc.