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Hipparcos trigonometric parallaxes and the distance scale for open star clusters. / Loktin, A.; Beshenov, G. V.
In: Astronomy Letters, Vol. 27, No. 6, 06.2001, p. 386-390.

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Harvard

Loktin, A & Beshenov, GV 2001, 'Hipparcos trigonometric parallaxes and the distance scale for open star clusters', Astronomy Letters, vol. 27, no. 6, pp. 386-390. https://doi.org/10.1134/1.1374677

APA

Loktin, A., & Beshenov, G. V. (2001). Hipparcos trigonometric parallaxes and the distance scale for open star clusters. Astronomy Letters, 27(6), 386-390. https://doi.org/10.1134/1.1374677

Vancouver

Loktin A, Beshenov GV. Hipparcos trigonometric parallaxes and the distance scale for open star clusters. Astronomy Letters. 2001 Jun;27(6):386-390. doi: 10.1134/1.1374677

Author

Loktin, A. ; Beshenov, G. V. / Hipparcos trigonometric parallaxes and the distance scale for open star clusters. In: Astronomy Letters. 2001 ; Vol. 27, No. 6. pp. 386-390.

BibTeX

@article{2c68b98dee9348358e4511da0b13b756,
title = "Hipparcos trigonometric parallaxes and the distance scale for open star clusters",
abstract = "Hipparcos trigonometric parallaxes are used to estimate the distances to the maximum possible number of open star clusters (OSC); distance moduli are estimated for 45 clusters with maximum heliocentric distances of about 1000 pc. The latter value can serve as an estimate of the limit to which it still makes sense to use Hipparcos trigonometric parallaxes to determine the distances to small groups composed of 6–10 sufficiently bright stars. A systematic correction to the distance moduli of clusters from the homogeneous catalog of OSC parameters (Loktin et al. 1997, 2000) is estimated, which turns out to be independent of the cluster age.",
author = "A. Loktin and Beshenov, {G. V.}",
year = "2001",
month = jun,
doi = "10.1134/1.1374677",
language = "English",
volume = "27",
pages = "386--390",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "Maik Nauka-Interperiodica Publishing",
number = "6",

}

RIS

TY - JOUR

T1 - Hipparcos trigonometric parallaxes and the distance scale for open star clusters

AU - Loktin, A.

AU - Beshenov, G. V.

PY - 2001/6

Y1 - 2001/6

N2 - Hipparcos trigonometric parallaxes are used to estimate the distances to the maximum possible number of open star clusters (OSC); distance moduli are estimated for 45 clusters with maximum heliocentric distances of about 1000 pc. The latter value can serve as an estimate of the limit to which it still makes sense to use Hipparcos trigonometric parallaxes to determine the distances to small groups composed of 6–10 sufficiently bright stars. A systematic correction to the distance moduli of clusters from the homogeneous catalog of OSC parameters (Loktin et al. 1997, 2000) is estimated, which turns out to be independent of the cluster age.

AB - Hipparcos trigonometric parallaxes are used to estimate the distances to the maximum possible number of open star clusters (OSC); distance moduli are estimated for 45 clusters with maximum heliocentric distances of about 1000 pc. The latter value can serve as an estimate of the limit to which it still makes sense to use Hipparcos trigonometric parallaxes to determine the distances to small groups composed of 6–10 sufficiently bright stars. A systematic correction to the distance moduli of clusters from the homogeneous catalog of OSC parameters (Loktin et al. 1997, 2000) is estimated, which turns out to be independent of the cluster age.

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U2 - 10.1134/1.1374677

DO - 10.1134/1.1374677

M3 - Article

VL - 27

SP - 386

EP - 390

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 6

ER -

ID: 42730405