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Is the late buckling stage inevitable in the bar life? / Smirnov, Anton A. ; Sotnikova, Natalia Ya. .

In: Monthly Notices of the Royal Astronomical Society, Vol. 485, No. 2, 2019, p. 1900-1905.

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

Harvard

Smirnov, AA & Sotnikova, NY 2019, 'Is the late buckling stage inevitable in the bar life?', Monthly Notices of the Royal Astronomical Society, vol. 485, no. 2, pp. 1900-1905. https://doi.org/10.1093/mnras/stz546

APA

Smirnov, A. A., & Sotnikova, N. Y. (2019). Is the late buckling stage inevitable in the bar life? Monthly Notices of the Royal Astronomical Society, 485(2), 1900-1905. https://doi.org/10.1093/mnras/stz546

Vancouver

Smirnov AA, Sotnikova NY. Is the late buckling stage inevitable in the bar life? Monthly Notices of the Royal Astronomical Society. 2019;485(2):1900-1905. https://doi.org/10.1093/mnras/stz546

Author

Smirnov, Anton A. ; Sotnikova, Natalia Ya. . / Is the late buckling stage inevitable in the bar life?. In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 485, No. 2. pp. 1900-1905.

BibTeX

@article{7aab4695d4384eb9a249ce8e07b3f6d3,
title = "Is the late buckling stage inevitable in the bar life?",
abstract = "By means of self-consistent numerical simulations we investigated the dynamical impact of classical bulges on the growth of the secondary buckling of a bar. Overall we considered 14 models with different disc and bulge parameters. We obtained that a bulge with a quite modest mass B/D = 0.1 leads to completely symmetrical evolution of the bar almost independently of the initial stellar disc parameters and even can damp the first bending. At the same time, the bars in all our bulgeless models suffer from the short primary and prolonged secondary buckling. Given the smallness of the mass suppressing secondary buckling, we conclude that a classical bulge along with the gas central concentration may be the main culprits for the rarity of bars with ongoing buckling in the local Universe.",
keywords = "galaxies: bulges, galaxies: evolution, galaxies: fundamental parameters, galaxies: general, galaxies: kinematics and dynamics, galaxies: structure, Galaxies: bulges, Galaxies: evolution, Galaxies: fundamental parameters, Galaxies: general, Galaxies: kinematics and dynamics, Galaxies: structure",
author = "Smirnov, {Anton A.} and Sotnikova, {Natalia Ya.}",
year = "2019",
doi = "https://doi.org/10.1093/mnras/stz546",
language = "English",
volume = "485",
pages = "1900--1905",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Wiley-Blackwell",
number = "2",

}

RIS

TY - JOUR

T1 - Is the late buckling stage inevitable in the bar life?

AU - Smirnov, Anton A.

AU - Sotnikova, Natalia Ya.

PY - 2019

Y1 - 2019

N2 - By means of self-consistent numerical simulations we investigated the dynamical impact of classical bulges on the growth of the secondary buckling of a bar. Overall we considered 14 models with different disc and bulge parameters. We obtained that a bulge with a quite modest mass B/D = 0.1 leads to completely symmetrical evolution of the bar almost independently of the initial stellar disc parameters and even can damp the first bending. At the same time, the bars in all our bulgeless models suffer from the short primary and prolonged secondary buckling. Given the smallness of the mass suppressing secondary buckling, we conclude that a classical bulge along with the gas central concentration may be the main culprits for the rarity of bars with ongoing buckling in the local Universe.

AB - By means of self-consistent numerical simulations we investigated the dynamical impact of classical bulges on the growth of the secondary buckling of a bar. Overall we considered 14 models with different disc and bulge parameters. We obtained that a bulge with a quite modest mass B/D = 0.1 leads to completely symmetrical evolution of the bar almost independently of the initial stellar disc parameters and even can damp the first bending. At the same time, the bars in all our bulgeless models suffer from the short primary and prolonged secondary buckling. Given the smallness of the mass suppressing secondary buckling, we conclude that a classical bulge along with the gas central concentration may be the main culprits for the rarity of bars with ongoing buckling in the local Universe.

KW - galaxies: bulges, galaxies: evolution, galaxies: fundamental parameters, galaxies: general, galaxies: kinematics and dynamics, galaxies: structure

KW - Galaxies: bulges

KW - Galaxies: evolution

KW - Galaxies: fundamental parameters

KW - Galaxies: general

KW - Galaxies: kinematics and dynamics

KW - Galaxies: structure

UR - http://www.scopus.com/inward/record.url?scp=85062837111&partnerID=8YFLogxK

U2 - https://doi.org/10.1093/mnras/stz546

DO - https://doi.org/10.1093/mnras/stz546

M3 - Article

VL - 485

SP - 1900

EP - 1905

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -

ID: 39419898