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The Praesepe open cluster and the galactic distance scale. / Loktin, A.
In: Astronomy Letters, Vol. 26, No. 10, 10.2000, p. 657-659.

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Harvard

Loktin, A 2000, 'The Praesepe open cluster and the galactic distance scale', Astronomy Letters, vol. 26, no. 10, pp. 657-659. https://doi.org/10.1134/1.1316110

APA

Loktin, A. (2000). The Praesepe open cluster and the galactic distance scale. Astronomy Letters, 26(10), 657-659. https://doi.org/10.1134/1.1316110

Vancouver

Loktin A. The Praesepe open cluster and the galactic distance scale. Astronomy Letters. 2000 Oct;26(10):657-659. doi: 10.1134/1.1316110

Author

Loktin, A. / The Praesepe open cluster and the galactic distance scale. In: Astronomy Letters. 2000 ; Vol. 26, No. 10. pp. 657-659.

BibTeX

@article{8663913734224b62a832bd1df28958e3,
title = "The Praesepe open cluster and the galactic distance scale",
abstract = "Updated proper motions for 328 probable members of the Praesepe are used to determine the distance to this open cluster by Hertzsprung's geometric method. The cluster distance was found to be r=171±15 pc, which corresponds to the distance modulus V0−MV=6.m16±0.19. The distance scale for open clusters is discussed.",
author = "A. Loktin",
year = "2000",
month = oct,
doi = "10.1134/1.1316110",
language = "English",
volume = "26",
pages = "657--659",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "Maik Nauka-Interperiodica Publishing",
number = "10",

}

RIS

TY - JOUR

T1 - The Praesepe open cluster and the galactic distance scale

AU - Loktin, A.

PY - 2000/10

Y1 - 2000/10

N2 - Updated proper motions for 328 probable members of the Praesepe are used to determine the distance to this open cluster by Hertzsprung's geometric method. The cluster distance was found to be r=171±15 pc, which corresponds to the distance modulus V0−MV=6.m16±0.19. The distance scale for open clusters is discussed.

AB - Updated proper motions for 328 probable members of the Praesepe are used to determine the distance to this open cluster by Hertzsprung's geometric method. The cluster distance was found to be r=171±15 pc, which corresponds to the distance modulus V0−MV=6.m16±0.19. The distance scale for open clusters is discussed.

UR - https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=tsmetrics&SrcApp=tsm_test&DestApp=WOS_CPL&DestLinkType=FullRecord&KeyUT=000090073600004

U2 - 10.1134/1.1316110

DO - 10.1134/1.1316110

M3 - Article

VL - 26

SP - 657

EP - 659

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 10

ER -

ID: 42730243