The formation of S0 galaxies with counter-rotating neutral and molecular hydrogen

Robert Bassett, Kenji Bekki, Luca Cortese, Warrick Couch

Research output: Contribution to journalArticle

Abstract

The observation of counter-rotation in galaxies (i.e. gas that rotates in the opposite direction to the stellar component or two cospatial stellar populations with opposite rotation) is becoming more commonplace with modern integral field spectroscopic surveys. In this paper, we explore the emergence of counter-rotation (both stellar and gaseous) in S0 galaxies from smoothedparticle hydrodynamics simulations of 1/10 mass ratio minor mergers between a similar to 10(10.8) M-circle dot disc galaxy with a bulge-to-total ratio of 0.17 and a gas-rich companion (gas-to-stellar mass fraction of 5.0). These simulations include a self-consistent treatment of gas dynamics, star formation, the production/destruction of H-2 and dust and the time evolution of the interstellar radiation field. We explore the effect of retrograde versus prograde obits, gas and bulge mass fractions of the primary galaxy, and orbital parameters of the companion. The key requirement for producing counter-rotation in stars or gas in a merger remnant is a retrograde primary, while the relative spin of the companion affects only the radial extent of the accreted gas. We also find that including a significant amount of gas in the primary can prevent the emergence of counter-rotating gas, although accreted stars retain counter-rotation. Bulge mass and orbit have a secondary effect, generally influencing the final distribution of accreted stars and gas within the framework outlined above. In addition to our primary focus of counter-rotating components in galaxies, we also make some predictions regarding the SFRs, H-2 distributions, and dust in minor-merger remnants.

LanguageEnglish
Pages1892-1909
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume471
Issue number2
DOIs
StatePublished - Oct 2017

Cite this

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title = "The formation of S0 galaxies with counter-rotating neutral and molecular hydrogen",
abstract = "The observation of counter-rotation in galaxies (i.e. gas that rotates in the opposite direction to the stellar component or two cospatial stellar populations with opposite rotation) is becoming more commonplace with modern integral field spectroscopic surveys. In this paper, we explore the emergence of counter-rotation (both stellar and gaseous) in S0 galaxies from smoothedparticle hydrodynamics simulations of 1/10 mass ratio minor mergers between a similar to 10(10.8) M-circle dot disc galaxy with a bulge-to-total ratio of 0.17 and a gas-rich companion (gas-to-stellar mass fraction of 5.0). These simulations include a self-consistent treatment of gas dynamics, star formation, the production/destruction of H-2 and dust and the time evolution of the interstellar radiation field. We explore the effect of retrograde versus prograde obits, gas and bulge mass fractions of the primary galaxy, and orbital parameters of the companion. The key requirement for producing counter-rotation in stars or gas in a merger remnant is a retrograde primary, while the relative spin of the companion affects only the radial extent of the accreted gas. We also find that including a significant amount of gas in the primary can prevent the emergence of counter-rotating gas, although accreted stars retain counter-rotation. Bulge mass and orbit have a secondary effect, generally influencing the final distribution of accreted stars and gas within the framework outlined above. In addition to our primary focus of counter-rotating components in galaxies, we also make some predictions regarding the SFRs, H-2 distributions, and dust in minor-merger remnants.",
keywords = "galaxies: interactions, galaxies: kinematics and dynamics, ACTIVE GALACTIC NUCLEI, STAR-FORMING GALAXIES, DIGITAL SKY SURVEY, COLD DARK-MATTER, ELLIPTIC GALAXIES, MERGER REMNANTS, BARRED GALAXIES, KINEMATIC SUBSYSTEMS, CHEMICAL EVOLUTION, ATLAS(3D) PROJECT",
author = "Robert Bassett and Kenji Bekki and Luca Cortese and Warrick Couch",
year = "2017",
month = "10",
doi = "10.1093/mnras/stx958",
language = "English",
volume = "471",
pages = "1892--1909",
journal = "Monthly Notices of the Royal Astronomical Society",
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The formation of S0 galaxies with counter-rotating neutral and molecular hydrogen. / Bassett, Robert; Bekki, Kenji; Cortese, Luca; Couch, Warrick.

In: Monthly Notices of the Royal Astronomical Society, Vol. 471, No. 2, 10.2017, p. 1892-1909.

Research output: Contribution to journalArticle

TY - JOUR

T1 - The formation of S0 galaxies with counter-rotating neutral and molecular hydrogen

AU - Bassett,Robert

AU - Bekki,Kenji

AU - Cortese,Luca

AU - Couch,Warrick

PY - 2017/10

Y1 - 2017/10

N2 - The observation of counter-rotation in galaxies (i.e. gas that rotates in the opposite direction to the stellar component or two cospatial stellar populations with opposite rotation) is becoming more commonplace with modern integral field spectroscopic surveys. In this paper, we explore the emergence of counter-rotation (both stellar and gaseous) in S0 galaxies from smoothedparticle hydrodynamics simulations of 1/10 mass ratio minor mergers between a similar to 10(10.8) M-circle dot disc galaxy with a bulge-to-total ratio of 0.17 and a gas-rich companion (gas-to-stellar mass fraction of 5.0). These simulations include a self-consistent treatment of gas dynamics, star formation, the production/destruction of H-2 and dust and the time evolution of the interstellar radiation field. We explore the effect of retrograde versus prograde obits, gas and bulge mass fractions of the primary galaxy, and orbital parameters of the companion. The key requirement for producing counter-rotation in stars or gas in a merger remnant is a retrograde primary, while the relative spin of the companion affects only the radial extent of the accreted gas. We also find that including a significant amount of gas in the primary can prevent the emergence of counter-rotating gas, although accreted stars retain counter-rotation. Bulge mass and orbit have a secondary effect, generally influencing the final distribution of accreted stars and gas within the framework outlined above. In addition to our primary focus of counter-rotating components in galaxies, we also make some predictions regarding the SFRs, H-2 distributions, and dust in minor-merger remnants.

AB - The observation of counter-rotation in galaxies (i.e. gas that rotates in the opposite direction to the stellar component or two cospatial stellar populations with opposite rotation) is becoming more commonplace with modern integral field spectroscopic surveys. In this paper, we explore the emergence of counter-rotation (both stellar and gaseous) in S0 galaxies from smoothedparticle hydrodynamics simulations of 1/10 mass ratio minor mergers between a similar to 10(10.8) M-circle dot disc galaxy with a bulge-to-total ratio of 0.17 and a gas-rich companion (gas-to-stellar mass fraction of 5.0). These simulations include a self-consistent treatment of gas dynamics, star formation, the production/destruction of H-2 and dust and the time evolution of the interstellar radiation field. We explore the effect of retrograde versus prograde obits, gas and bulge mass fractions of the primary galaxy, and orbital parameters of the companion. The key requirement for producing counter-rotation in stars or gas in a merger remnant is a retrograde primary, while the relative spin of the companion affects only the radial extent of the accreted gas. We also find that including a significant amount of gas in the primary can prevent the emergence of counter-rotating gas, although accreted stars retain counter-rotation. Bulge mass and orbit have a secondary effect, generally influencing the final distribution of accreted stars and gas within the framework outlined above. In addition to our primary focus of counter-rotating components in galaxies, we also make some predictions regarding the SFRs, H-2 distributions, and dust in minor-merger remnants.

KW - galaxies: interactions

KW - galaxies: kinematics and dynamics

KW - ACTIVE GALACTIC NUCLEI

KW - STAR-FORMING GALAXIES

KW - DIGITAL SKY SURVEY

KW - COLD DARK-MATTER

KW - ELLIPTIC GALAXIES

KW - MERGER REMNANTS

KW - BARRED GALAXIES

KW - KINEMATIC SUBSYSTEMS

KW - CHEMICAL EVOLUTION

KW - ATLAS(3D) PROJECT

U2 - 10.1093/mnras/stx958

DO - 10.1093/mnras/stx958

M3 - Article

VL - 471

SP - 1892

EP - 1909

JO - Monthly Notices of the Royal Astronomical Society

T2 - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -