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Luminosity calibration for OB stars from Hipparcos trigonometric parallaxes. / Loktin, A.; Beshenov, G.
In: Astronomy Reports, Vol. 45, No. 9, 01.09.2001, p. 711-717.

Research output: Contribution to journal › Article › peer-review

Harvard

Loktin, A & Beshenov, G 2001, 'Luminosity calibration for OB stars from Hipparcos trigonometric parallaxes', Astronomy Reports, vol. 45, no. 9, pp. 711-717. https://doi.org/10.1134/1.1398920

APA

Loktin, A., & Beshenov, G. (2001). Luminosity calibration for OB stars from Hipparcos trigonometric parallaxes. Astronomy Reports, 45(9), 711-717. https://doi.org/10.1134/1.1398920

Vancouver

Loktin A, Beshenov G. Luminosity calibration for OB stars from Hipparcos trigonometric parallaxes. Astronomy Reports. 2001 Sept 1;45(9):711-717. doi: 10.1134/1.1398920

Author

Loktin, A. ; Beshenov, G. / Luminosity calibration for OB stars from Hipparcos trigonometric parallaxes. In: Astronomy Reports. 2001 ; Vol. 45, No. 9. pp. 711-717.

BibTeX

@article{da5cdc4471284227889858dd0a4b4b81,
title = "Luminosity calibration for OB stars from Hipparcos trigonometric parallaxes",
abstract = "Hipparcos trigonometric parallaxes and observational data for open clusters are used to determine the absolute magnitudes M V of O and B stars of various spectral subtypes and luminosity classes, including those with broadened lines and hydrogen emission lines. The same data are used to derive a relation between M V and the index β of the Str{\"o}mgren photometric system. The resulting calibrations and the spectroscopic-parallax method are used to determine the distances to young open clusters.",
author = "A. Loktin and G. Beshenov",
year = "2001",
month = sep,
day = "1",
doi = "10.1134/1.1398920",
language = "English",
volume = "45",
pages = "711--717",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "Pleiades Publishing",
number = "9",

}

RIS

TY - JOUR

T1 - Luminosity calibration for OB stars from Hipparcos trigonometric parallaxes

AU - Loktin, A.

AU - Beshenov, G.

PY - 2001/9/1

Y1 - 2001/9/1

N2 - Hipparcos trigonometric parallaxes and observational data for open clusters are used to determine the absolute magnitudes M V of O and B stars of various spectral subtypes and luminosity classes, including those with broadened lines and hydrogen emission lines. The same data are used to derive a relation between M V and the index β of the Strömgren photometric system. The resulting calibrations and the spectroscopic-parallax method are used to determine the distances to young open clusters.

AB - Hipparcos trigonometric parallaxes and observational data for open clusters are used to determine the absolute magnitudes M V of O and B stars of various spectral subtypes and luminosity classes, including those with broadened lines and hydrogen emission lines. The same data are used to derive a relation between M V and the index β of the Strömgren photometric system. The resulting calibrations and the spectroscopic-parallax method are used to determine the distances to young open clusters.

UR - https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=tsmetrics&SrcApp=tsm_test&DestApp=WOS_CPL&DestLinkType=FullRecord&KeyUT=000171198700006

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=0035538025

U2 - 10.1134/1.1398920

DO - 10.1134/1.1398920

M3 - Article

VL - 45

SP - 711

EP - 717

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 9

ER -

ID: 42967826