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Determination of distances to galaxies by the brightest stars. / Tikhonov, N. A.; Galazutdinova, O. A.; Karataeva, G. .

в: Proceedings of Science, Том 425, 14.12.2022.

Результаты исследований: Научные публикации в периодических изданиях › статья в журнале по материалам конференции › Рецензирование

Harvard

Tikhonov, NA, Galazutdinova, OA & Karataeva, G 2022, 'Determination of distances to galaxies by the brightest stars', Proceedings of Science, Том. 425. https://doi.org/10.22323/1.425.0021

APA

Tikhonov, N. A., Galazutdinova, O. A., & Karataeva, G. (2022). Determination of distances to galaxies by the brightest stars. Proceedings of Science, 425. https://doi.org/10.22323/1.425.0021

Vancouver

Tikhonov NA, Galazutdinova OA, Karataeva G. Determination of distances to galaxies by the brightest stars. Proceedings of Science. 2022 Дек. 14;425. https://doi.org/10.22323/1.425.0021

Author

Tikhonov, N. A. ; Galazutdinova, O. A. ; Karataeva, G. . / Determination of distances to galaxies by the brightest stars. в: Proceedings of Science. 2022 ; Том 425.

BibTeX

@article{1ea79265b1e3462598e6076744a2ff93,
title = "Determination of distances to galaxies by the brightest stars",
abstract = "Currently, the common method for determining the distances to galaxies for red giants (TRGB method) has a measurement limit of approximately 25~Mpc. In more distant galaxies, red giants are not visible in images of Hubble Space Telescope (HST). For such galaxies, we propose to use the already well-known method of the brightest stars, calibrated by us on the basis of HST telescope images for 150 galaxies of different types and luminosities. The obtained relationship between the luminosities of galaxies and their brightest stars can be used for irregular and spiral galaxies in a large span of their luminosities ranged from MB=−8m to MB=−19m . Because the brightest stars have a luminosity 4--5 magnitudes higher than the luminosity of red giants, the method of the brightest stars can be applied for significantly more distant galaxies. The accuracy of the brightest blue star method is 0.m4.",
author = "Tikhonov, {N. A.} and Galazutdinova, {O. A.} and G. Karataeva",
note = "2022muto.confE..21T; The Multifaceted Universe: Theory and Observations - 2022 : 23-27 May 2022 SAO RAS, Nizhny Arkhyz, Russia ; Conference date: 23-05-2022",
year = "2022",
month = dec,
day = "14",
doi = "10.22323/1.425.0021",
language = "English",
volume = "425",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",

}

RIS

TY - JOUR

T1 - Determination of distances to galaxies by the brightest stars

AU - Tikhonov, N. A.

AU - Galazutdinova, O. A.

AU - Karataeva, G.

N1 - 2022muto.confE..21T

PY - 2022/12/14

Y1 - 2022/12/14

N2 - Currently, the common method for determining the distances to galaxies for red giants (TRGB method) has a measurement limit of approximately 25~Mpc. In more distant galaxies, red giants are not visible in images of Hubble Space Telescope (HST). For such galaxies, we propose to use the already well-known method of the brightest stars, calibrated by us on the basis of HST telescope images for 150 galaxies of different types and luminosities. The obtained relationship between the luminosities of galaxies and their brightest stars can be used for irregular and spiral galaxies in a large span of their luminosities ranged from MB=−8m to MB=−19m . Because the brightest stars have a luminosity 4--5 magnitudes higher than the luminosity of red giants, the method of the brightest stars can be applied for significantly more distant galaxies. The accuracy of the brightest blue star method is 0.m4.

AB - Currently, the common method for determining the distances to galaxies for red giants (TRGB method) has a measurement limit of approximately 25~Mpc. In more distant galaxies, red giants are not visible in images of Hubble Space Telescope (HST). For such galaxies, we propose to use the already well-known method of the brightest stars, calibrated by us on the basis of HST telescope images for 150 galaxies of different types and luminosities. The obtained relationship between the luminosities of galaxies and their brightest stars can be used for irregular and spiral galaxies in a large span of their luminosities ranged from MB=−8m to MB=−19m . Because the brightest stars have a luminosity 4--5 magnitudes higher than the luminosity of red giants, the method of the brightest stars can be applied for significantly more distant galaxies. The accuracy of the brightest blue star method is 0.m4.

U2 - 10.22323/1.425.0021

DO - 10.22323/1.425.0021

M3 - Conference article

VL - 425

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

T2 - The Multifaceted Universe: Theory and Observations - 2022

Y2 - 23 May 2022

ER -

ID: 103073177