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Comparison of the luminosity functions of open clusters based on USNO-A1 data. / Zakharova, P. E.; Loktin, A. V.
в: Astronomy Reports, Том 48, № 9, 01.09.2004, стр. 733-741.

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Harvard

Zakharova, PE & Loktin, AV 2004, 'Comparison of the luminosity functions of open clusters based on USNO-A1 data', Astronomy Reports, Том. 48, № 9, стр. 733-741. https://doi.org/10.1134/1.1800173

APA

Zakharova, P. E., & Loktin, A. V. (2004). Comparison of the luminosity functions of open clusters based on USNO-A1 data. Astronomy Reports, 48(9), 733-741. https://doi.org/10.1134/1.1800173

Vancouver

Zakharova PE, Loktin AV. Comparison of the luminosity functions of open clusters based on USNO-A1 data. Astronomy Reports. 2004 сент. 1;48(9):733-741. doi: 10.1134/1.1800173

Author

Zakharova, P. E. ; Loktin, A. V. / Comparison of the luminosity functions of open clusters based on USNO-A1 data. в: Astronomy Reports. 2004 ; Том 48, № 9. стр. 733-741.

BibTeX

@article{4ba3d09f15be440096086172aa00b021,
title = "Comparison of the luminosity functions of open clusters based on USNO-A1 data",
abstract = "The luminosity and mass functions of a group of Galactic open clusters are constructed by applying a statistical method to photometric data from the USNO-A1 catalog. Despite some limitations, this catalog can be used for statistical analyses in Galactic astronomy. Pairwise comparisons of the derived cluster luminosity functions are performed for five age intervals. The differences between the luminosity functions of the open clusters are not statistically significant in most cases. It is concluded that the luminosity functions are approximately universal throughout a large volume in the solar neighborhood. Combined luminosity and mass functions are constructed for six age intervals. The slope of the mass spectrum may vary somewhat from cluster to cluster, and the mean slope may be somewhat higher than the Salpeter value.",
author = "Zakharova, {P. E.} and Loktin, {A. V.}",
note = "This work was supported by the Russian Foundation for Basic Research (project no. 00-02-16217).",
year = "2004",
month = sep,
day = "1",
doi = "10.1134/1.1800173",
language = "English",
volume = "48",
pages = "733--741",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "Pleiades Publishing",
number = "9",

}

RIS

TY - JOUR

T1 - Comparison of the luminosity functions of open clusters based on USNO-A1 data

AU - Zakharova, P. E.

AU - Loktin, A. V.

N1 - This work was supported by the Russian Foundation for Basic Research (project no. 00-02-16217).

PY - 2004/9/1

Y1 - 2004/9/1

N2 - The luminosity and mass functions of a group of Galactic open clusters are constructed by applying a statistical method to photometric data from the USNO-A1 catalog. Despite some limitations, this catalog can be used for statistical analyses in Galactic astronomy. Pairwise comparisons of the derived cluster luminosity functions are performed for five age intervals. The differences between the luminosity functions of the open clusters are not statistically significant in most cases. It is concluded that the luminosity functions are approximately universal throughout a large volume in the solar neighborhood. Combined luminosity and mass functions are constructed for six age intervals. The slope of the mass spectrum may vary somewhat from cluster to cluster, and the mean slope may be somewhat higher than the Salpeter value.

AB - The luminosity and mass functions of a group of Galactic open clusters are constructed by applying a statistical method to photometric data from the USNO-A1 catalog. Despite some limitations, this catalog can be used for statistical analyses in Galactic astronomy. Pairwise comparisons of the derived cluster luminosity functions are performed for five age intervals. The differences between the luminosity functions of the open clusters are not statistically significant in most cases. It is concluded that the luminosity functions are approximately universal throughout a large volume in the solar neighborhood. Combined luminosity and mass functions are constructed for six age intervals. The slope of the mass spectrum may vary somewhat from cluster to cluster, and the mean slope may be somewhat higher than the Salpeter value.

UR - https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=tsmetrics&SrcApp=tsm_test&DestApp=WOS_CPL&DestLinkType=FullRecord&KeyUT=000224310200005

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=7444256803

U2 - 10.1134/1.1800173

DO - 10.1134/1.1800173

M3 - Article

VL - 48

SP - 733

EP - 741

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 9

ER -

ID: 43967888