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Resolution of the observed dispersion of the radial velocities of a galactic subsystem into components. / Nikiforov, I. I.

In: Astrophysics, Vol. 43, No. 3, 01.01.2000, p. 322-327.

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

Harvard

Nikiforov, II 2000, 'Resolution of the observed dispersion of the radial velocities of a galactic subsystem into components', Astrophysics, vol. 43, no. 3, pp. 322-327. https://doi.org/10.1007/BF02683967

APA

Nikiforov, I. I. (2000). Resolution of the observed dispersion of the radial velocities of a galactic subsystem into components. Astrophysics, 43(3), 322-327. https://doi.org/10.1007/BF02683967

Vancouver

Nikiforov II. Resolution of the observed dispersion of the radial velocities of a galactic subsystem into components. Astrophysics. 2000 Jan 1;43(3):322-327. https://doi.org/10.1007/BF02683967

Author

Nikiforov, I. I. / Resolution of the observed dispersion of the radial velocities of a galactic subsystem into components. In: Astrophysics. 2000 ; Vol. 43, No. 3. pp. 322-327.

BibTeX

@article{675241fe9c53498d889b9837a8d77ba8,
title = "Resolution of the observed dispersion of the radial velocities of a galactic subsystem into components",
abstract = "Possible approaches are considered to the problem of resolving the observed dispersion in the radial velocities of objects of a given kind in the Galaxy into the system's true dispersion and the contribution of random errors in heliocentric distances r. Of the methods that have been constructed, only the joint estimation of the true dispersion and the relative mean error in r can yield satisfactory results. This method is used for the subsystem of CO clouds with an observed dispersion of 8.7 ± 0.4 km/sec to obtain the true dispersion of 8.0 ± 0.6 km/sec and the mean error of 0m.25 ± 0m.085 in their distance moduli.",
author = "Nikiforov, {I. I.}",
note = "Перевод статьи {"}Разложение на составляющие наблюдаемой дисперсии лучевых скоростей галактической подсистемы{"}, Никифоров, И. И., 2000, в : АСТРОФИЗИКА. 43, Вып. 3, стр. 443-450",
year = "2000",
month = jan,
day = "1",
doi = "10.1007/BF02683967",
language = "English",
volume = "43",
pages = "322--327",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "3",

}

RIS

TY - JOUR

T1 - Resolution of the observed dispersion of the radial velocities of a galactic subsystem into components

AU - Nikiforov, I. I.

N1 - Перевод статьи "Разложение на составляющие наблюдаемой дисперсии лучевых скоростей галактической подсистемы", Никифоров, И. И., 2000, в : АСТРОФИЗИКА. 43, Вып. 3, стр. 443-450

PY - 2000/1/1

Y1 - 2000/1/1

N2 - Possible approaches are considered to the problem of resolving the observed dispersion in the radial velocities of objects of a given kind in the Galaxy into the system's true dispersion and the contribution of random errors in heliocentric distances r. Of the methods that have been constructed, only the joint estimation of the true dispersion and the relative mean error in r can yield satisfactory results. This method is used for the subsystem of CO clouds with an observed dispersion of 8.7 ± 0.4 km/sec to obtain the true dispersion of 8.0 ± 0.6 km/sec and the mean error of 0m.25 ± 0m.085 in their distance moduli.

AB - Possible approaches are considered to the problem of resolving the observed dispersion in the radial velocities of objects of a given kind in the Galaxy into the system's true dispersion and the contribution of random errors in heliocentric distances r. Of the methods that have been constructed, only the joint estimation of the true dispersion and the relative mean error in r can yield satisfactory results. This method is used for the subsystem of CO clouds with an observed dispersion of 8.7 ± 0.4 km/sec to obtain the true dispersion of 8.0 ± 0.6 km/sec and the mean error of 0m.25 ± 0m.085 in their distance moduli.

UR - http://www.scopus.com/inward/record.url?scp=52849099641&partnerID=8YFLogxK

U2 - 10.1007/BF02683967

DO - 10.1007/BF02683967

M3 - Article

AN - SCOPUS:52849099641

VL - 43

SP - 322

EP - 327

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 3

ER -

ID: 35704581