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Evolution of the Structure of Edge-On Spiral Galaxies. / Решетников, Владимир Петрович; Усачев, Павел Александрович.

в: Astrophysics, Том 64, № 1, 02.2021, стр. 1-7.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

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@article{bfa455fd667345f4b7ffb607602ca45f,
title = "Evolution of the Structure of Edge-On Spiral Galaxies",
abstract = "The results of a photometric analysis of edge-on spiral galaxies in three blue fields of the Hubble Space Telescope (HDF-N, FDF-S, HUDF) are discussed. It is shown that galaxies at z ≈ 0.5 have lower values of the radial exponential scales h r of the stellar disks compared to nearby galaxies. The observed variation in the scales of the disks is consistent with a n h r ∝ (1 + z) –n law, where n ≈ 1. Indications are found of a significant reduction in the fraction of galaxies with B/PS bulges from z=0 to z=1. ",
keywords = "evolution of structure, spiral galaxies",
author = "Решетников, {Владимир Петрович} and Усачев, {Павел Александрович}",
year = "2021",
month = feb,
doi = "10.1007/s10511-021-09662-7",
language = "English",
volume = "64",
pages = "1--7",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "1",

}

RIS

TY - JOUR

T1 - Evolution of the Structure of Edge-On Spiral Galaxies

AU - Решетников, Владимир Петрович

AU - Усачев, Павел Александрович

PY - 2021/2

Y1 - 2021/2

N2 - The results of a photometric analysis of edge-on spiral galaxies in three blue fields of the Hubble Space Telescope (HDF-N, FDF-S, HUDF) are discussed. It is shown that galaxies at z ≈ 0.5 have lower values of the radial exponential scales h r of the stellar disks compared to nearby galaxies. The observed variation in the scales of the disks is consistent with a n h r ∝ (1 + z) –n law, where n ≈ 1. Indications are found of a significant reduction in the fraction of galaxies with B/PS bulges from z=0 to z=1.

AB - The results of a photometric analysis of edge-on spiral galaxies in three blue fields of the Hubble Space Telescope (HDF-N, FDF-S, HUDF) are discussed. It is shown that galaxies at z ≈ 0.5 have lower values of the radial exponential scales h r of the stellar disks compared to nearby galaxies. The observed variation in the scales of the disks is consistent with a n h r ∝ (1 + z) –n law, where n ≈ 1. Indications are found of a significant reduction in the fraction of galaxies with B/PS bulges from z=0 to z=1.

KW - evolution of structure

KW - spiral galaxies

UR - http://www.scopus.com/inward/record.url?scp=85102335305&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/38ae9218-7772-3469-ad40-bbababa6c424/

U2 - 10.1007/s10511-021-09662-7

DO - 10.1007/s10511-021-09662-7

M3 - Article

VL - 64

SP - 1

EP - 7

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 1

ER -

ID: 74814873