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Galaxy masses
Galaxy masses play a fundamental role in our understanding of structure formation models.
This review addresses the variety and reliability of mass estimators that pertain to stars, gas …
This review addresses the variety and reliability of mass estimators that pertain to stars, gas …
A review of recent observations of galactic winds driven by star formation
Galaxy-scale outflows of gas, or galactic winds (GWs), driven by energy from star formation
are a pivotal mechanism for regulation of star formation in the current model of galaxy …
are a pivotal mechanism for regulation of star formation in the current model of galaxy …
Overview of the SDSS-IV MaNGA survey: map** nearby galaxies at Apache Point observatory
We present an overview of a new integral field spectroscopic survey called MaNGA
(Map** Nearby Galaxies at Apache Point Observatory), one of three core programs in the …
(Map** Nearby Galaxies at Apache Point Observatory), one of three core programs in the …
The unexpected diversity of dwarf galaxy rotation curves
We examine the circular velocity profiles of galaxies in Λ cold dark matter (CDM)
cosmological hydrodynamical simulations from the EAGLE and LOCAL GROUPS projects …
cosmological hydrodynamical simulations from the EAGLE and LOCAL GROUPS projects …
Baryon effects on the internal structure of ΛCDM haloes in the EAGLE simulations
We investigate the internal structure and density profiles of haloes of mass 1010–1014 M⊙
in the Evolution and Assembly of Galaxies and their Environment (EAGLE) simulations …
in the Evolution and Assembly of Galaxies and their Environment (EAGLE) simulations …
The baryonic Tully–Fisher relation for different velocity definitions and implications for galaxy angular momentum
We study the baryonic Tully–Fisher relation (BTFR) at z≃ 0 using 153 galaxies from the
Spitzer Photometry and Accurate Rotation Curve sample. We consider different definitions of …
Spitzer Photometry and Accurate Rotation Curve sample. We consider different definitions of …
Making Galaxies In a Cosmological Context: the need for early stellar feedback
Abstract We introduce the Making Galaxies In a Cosmological Context (MAGICC)
programme of smoothed particle hydrodynamics simulations. We describe a parameter …
programme of smoothed particle hydrodynamics simulations. We describe a parameter …
Observations of feedback from radio-quiet quasars–II. Kinematics of ionized gas nebulae
The prevalence and energetics of quasar feedback is a major unresolved problem in galaxy
formation theory. In this paper, we present Gemini Integral Field Unit observations of ionized …
formation theory. In this paper, we present Gemini Integral Field Unit observations of ionized …
Characterizing Extreme Emission-line Galaxies. I. A Four-zone Ionization Model for Very High-ionization Emission
Stellar population models produce radiation fields that ionize oxygen up to O+ 2, defining
the limit of standard H ii region models (< 54.9 eV). Yet, some extreme emission-line …
the limit of standard H ii region models (< 54.9 eV). Yet, some extreme emission-line …
A model for cosmological simulations of galaxy formation physics: multi-epoch validation
We present a multi-epoch analysis of the galaxy populations formed within the cosmological
hydrodynamical simulations presented in Vogelsberger et al. These simulations explore the …
hydrodynamical simulations presented in Vogelsberger et al. These simulations explore the …