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The luminosity function of ringed galaxies. / Smirnov, Daniil V. ; Reshetnikov, Vladimir P. .

In: Monthly Notices of the Royal Astronomical Society, Vol. 516, No. 3, 09.2022, p. 3692-3700.

Research output: Contribution to journalArticlepeer-review

Harvard

Smirnov, DV & Reshetnikov, VP 2022, 'The luminosity function of ringed galaxies', Monthly Notices of the Royal Astronomical Society, vol. 516, no. 3, pp. 3692-3700. https://doi.org/10.1093/mnras/stac2549

APA

Smirnov, D. V., & Reshetnikov, V. P. (2022). The luminosity function of ringed galaxies. Monthly Notices of the Royal Astronomical Society, 516(3), 3692-3700. https://doi.org/10.1093/mnras/stac2549

Vancouver

Smirnov DV, Reshetnikov VP. The luminosity function of ringed galaxies. Monthly Notices of the Royal Astronomical Society. 2022 Sep;516(3):3692-3700. https://doi.org/10.1093/mnras/stac2549

Author

Smirnov, Daniil V. ; Reshetnikov, Vladimir P. . / The luminosity function of ringed galaxies. In: Monthly Notices of the Royal Astronomical Society. 2022 ; Vol. 516, No. 3. pp. 3692-3700.

BibTeX

@article{3905f5d58b244658abfd603681afc571,
title = "The luminosity function of ringed galaxies",
abstract = "We perform an analysis of the luminosity functions (LFs) of two types of ringed galaxies – polar-ring galaxies and collisional ring galaxies – using data from the Sloan Digital Sky Survey (SDSS). Both classes of galaxies were formed as a result of interaction with their environment and they are very rare objects. We constructed LFs of galaxies by different methods and found their approximations by the Schechter function. The luminosity functions of both types of galaxies show a systematic fall-off at low luminosities. The polar structures around bright (Mr ≤ −20m) and red (g − r > +0.8) galaxies are about twice as common as around blue ones. The LF of collisional rings is shifted towards brighter luminosities compared to polar-ring galaxies. We analysed the published data on the ringed galaxies in several deep fields and confirmed the increase in their volume density with redshift: up to z ∼ 1 their density grows as (1 + z)m, where m ≳ 5.",
keywords = "galaxies: evolution, galaxies: interactions, galaxies: peculiar, Galaxies: statistics",
author = "Smirnov, {Daniil V.} and Reshetnikov, {Vladimir P.}",
year = "2022",
month = sep,
doi = "10.1093/mnras/stac2549",
language = "English",
volume = "516",
pages = "3692--3700",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Wiley-Blackwell",
number = "3",

}

RIS

TY - JOUR

T1 - The luminosity function of ringed galaxies

AU - Smirnov, Daniil V.

AU - Reshetnikov, Vladimir P.

PY - 2022/9

Y1 - 2022/9

N2 - We perform an analysis of the luminosity functions (LFs) of two types of ringed galaxies – polar-ring galaxies and collisional ring galaxies – using data from the Sloan Digital Sky Survey (SDSS). Both classes of galaxies were formed as a result of interaction with their environment and they are very rare objects. We constructed LFs of galaxies by different methods and found their approximations by the Schechter function. The luminosity functions of both types of galaxies show a systematic fall-off at low luminosities. The polar structures around bright (Mr ≤ −20m) and red (g − r > +0.8) galaxies are about twice as common as around blue ones. The LF of collisional rings is shifted towards brighter luminosities compared to polar-ring galaxies. We analysed the published data on the ringed galaxies in several deep fields and confirmed the increase in their volume density with redshift: up to z ∼ 1 their density grows as (1 + z)m, where m ≳ 5.

AB - We perform an analysis of the luminosity functions (LFs) of two types of ringed galaxies – polar-ring galaxies and collisional ring galaxies – using data from the Sloan Digital Sky Survey (SDSS). Both classes of galaxies were formed as a result of interaction with their environment and they are very rare objects. We constructed LFs of galaxies by different methods and found their approximations by the Schechter function. The luminosity functions of both types of galaxies show a systematic fall-off at low luminosities. The polar structures around bright (Mr ≤ −20m) and red (g − r > +0.8) galaxies are about twice as common as around blue ones. The LF of collisional rings is shifted towards brighter luminosities compared to polar-ring galaxies. We analysed the published data on the ringed galaxies in several deep fields and confirmed the increase in their volume density with redshift: up to z ∼ 1 their density grows as (1 + z)m, where m ≳ 5.

KW - galaxies: evolution

KW - galaxies: interactions

KW - galaxies: peculiar

KW - Galaxies: statistics

UR - https://www.mendeley.com/catalogue/17f69dad-4e0e-38fd-be19-5977db361610/

U2 - 10.1093/mnras/stac2549

DO - 10.1093/mnras/stac2549

M3 - Article

VL - 516

SP - 3692

EP - 3700

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -

ID: 98907220