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The first spectroscopically confirmed Mira star in M33
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SYSNO ASEP 0367903 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title The first spectroscopically confirmed Mira star in M33 Author(s) Barsukova, E.A. (RU)
Goranskij, V.P. (RU)
Hornoch, Kamil (ASU-R) ORCID
Fabrika, S. (RU)
Pietsch, W. (DE)
Sholukhova, O. (RU)
Valeev, A.F. (RU)Source Title Monthly Notices of the Royal Astronomical Society. - : Oxford University Press - ISSN 0035-8711
Roč. 413, č. 3 (2011), s. 1797-1802Number of pages 6 s. Language eng - English Country GB - United Kingdom Keywords AGB and post AGB ; variables stars ; general galaxies Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000290487700026 DOI 10.1111/j.1365-2966.2011.18255.x Annotation Abstract We present photometry and moderate-resolution spectroscopy of the luminous red variable [HBS 2006] 40671, originally detected as a possible nova in the galaxy M33. We find that the star is a pulsating Mira-type variable with a long period of 665 d and an amplitude exceeding 7 mag in the R band. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2012
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