The first spectroscopically confirmed Mira star in M33
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F11%3A00367903" target="_blank" >RIV/67985815:_____/11:00367903 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1111/j.1365-2966.2011.18255.x" target="_blank" >http://dx.doi.org/10.1111/j.1365-2966.2011.18255.x</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1111/j.1365-2966.2011.18255.x" target="_blank" >10.1111/j.1365-2966.2011.18255.x</a>
Alternative languages
Result language
angličtina
Original language name
The first spectroscopically confirmed Mira star in M33
Original language description
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 665d and an amplitude exceeding 7 mag in the R band.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2011
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Monthly Notices of the Royal Astronomical Society
ISSN
0035-8711
e-ISSN
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Volume of the periodical
413
Issue of the periodical within the volume
3
Country of publishing house
GB - UNITED KINGDOM
Number of pages
6
Pages from-to
1797-1802
UT code for WoS article
000290487700026
EID of the result in the Scopus database
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