The Pulsation of $i$ Cygni Imaged by Optical Interferometry: A Novel Technique to Derive Distance and Mass of Mira Stars

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

Research output: Contribution to journalArticle

28 Citations (Scopus)
Original languageUndefined/Unknown
Pages (from-to)632-643
Number of pages12
JournalAstrophysical Journal
Volume707
Issue number1
DOIs
Publication statusPublished - 24 Nov 2009

Keywords

  • infrared: stars, stars: AGB and post-AGB, stars: fundamental parameters, stars: individual: chi Cyg, techniques: interferometric

Cite this

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. (2009). The Pulsation of $i$ Cygni Imaged by Optical Interferometry: A Novel Technique to Derive Distance and Mass of Mira Stars. Astrophysical Journal, 707(1), 632-643. https://doi.org/10.1088/0004-637X/707/1/632