THE PULSATION OF χ CYGNI IMAGED BY OPTICAL INTERFEROMETRY: A NOVEL TECHNIQUE TO DERIVE DISTANCE AND MASS OF MIRA STARS-Reference-Cited by-同舟云学术

THE PULSATION OF χ CYGNI IMAGED BY OPTICAL INTERFEROMETRY: A NOVEL TECHNIQUE TO DERIVE DISTANCE AND MASS OF MIRA STARS

Published:2009-11-24 Issue:1 Volume:707 Page:632-643
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Lacour S.,Thiébaut E.,Perrin G.,Meimon S.,Haubois X.,Pedretti E.,Ridgway S. T.,Monnier J. D.,Berger J. P.,Schuller P. A.,Woodruff H.,Poncelet A.,Le Coroller H.,Millan-Gabet R.,Lacasse M.,Traub W.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference74 articles.

1. Phase-dependent Variation of the Fundamental Parameters of Cepheids. III. Periods between 3 and 6 Days

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3. An integrated-optics 3-way beam combiner for IOTA

4. A periodic shock wave model for Mira variable atmospheres

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