VELČOVSKÝ, Jaroslav a Jan JANÍK. Complex study of the open cluster NGC 2281. In Alejandra Recio-Blanco, Patrick de Laverny, Anthony G. A. Brown, Timo Prusti. Astrometry and astrophysics in the Gaia sky. Glasgow (UK): Cambridge University Press. s. 273-274. ISBN 978-1-107-17008-7. doi:10.1017/S1743921317005993. 2018.
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Základní údaje
Originální název Complex study of the open cluster NGC 2281
Název česky Komplexní studie otevřené hvězdokupy NGC 2281
Autoři VELČOVSKÝ, Jaroslav (203 Česká republika, domácí) a Jan JANÍK (203 Česká republika, garant, domácí).
Vydání Glasgow (UK), Astrometry and astrophysics in the Gaia sky, od s. 273-274, 2 s. 2018.
Nakladatel Cambridge University Press
Další údaje
Originální jazyk angličtina
Typ výsledku Stať ve sborníku
Obor 10308 Astronomy
Stát vydavatele Velká Británie a Severní Irsko
Utajení není předmětem státního či obchodního tajemství
Forma vydání tištěná verze "print"
Kód RIV RIV/00216224:14310/18:00102439
Organizační jednotka Přírodovědecká fakulta
ISBN 978-1-107-17008-7
ISSN 1743-9213
Doi http://dx.doi.org/10.1017/S1743921317005993
UT WoS 000454738700075
Klíčová slova česky complex study; NGC 2281; membership probability
Klíčová slova anglicky complex study; NGC 2281; membership probability
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnil: RNDr. Jan Janík, Ph.D., učo 17241. Změněno: 25. 3. 2019 14:28.
Anotace
We present the complex study of the open cluster NGC 2281 where both traditional and newly developed methods for study of open clusters have been used. Morphological and dynamical parameters of the cluster were obtained from the accepted astrometric data. The new method “Superposition of Gaussian surfaces” along with proper motion of stars was used to determine membership probabilities which were helpful in selection of stars for further analysis. Metallicity and radial velocity of the cluster were obtained from spectroscopic measurements. Age, colour excess, and distance of the cluster were determined using absolute CCD photometry combined with previous results. The results were compared with those of previous studies.
Anotace česky
We present the complex study of the open cluster NGC 2281 where both traditional and newly developed methods for study of open clusters have been used. Morphological and dynamical parameters of the cluster were obtained from the accepted astrometric data. The new method “Superposition of Gaussian surfaces” along with proper motion of stars was used to determine membership probabilities which were helpful in selection of stars for further analysis. Metallicity and radial velocity of the cluster were obtained from spectroscopic measurements. Age, colour excess, and distance of the cluster were determined using absolute CCD photometry combined with previous results. The results were compared with those of previous studies.
VytisknoutZobrazeno: 20. 4. 2024 07:57