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Merger Signatures in the Dynamics of Star-forming Gas
Chao-Ling Hung, Christopher C. Hayward, Howard A. Smith +5
Spatially resolved kinematics have been used to determine the dynamical status of star-forming galaxies with ambiguous morphologies, and constrain the importance of galaxy interact…
How stellar feedback simultaneously regulates star formation and drives outflows
Christopher C. Hayward, Philip F. Hopkins
We present an analytic model for how momentum deposition from stellar feedback simultaneously regulates star formation and drives outflows in a turbulent interstellar medium (ISM).…
(Star)bursts of FIRE: observational signatures of bursty star formation in galaxies
Martin Sparre, Christopher C. Hayward, Robert Feldmann +4
Galaxy formation models are now able to reproduce observed relations such as the relation between galaxies' star formation rates (SFRs) and stellar masses () and the stellar m…
The Formation of Submillimetre-Bright Galaxies from Gas Infall over a Billion Years
Desika Narayanan, Matthew Turk, Robert Feldmann +7
Submillimetre-luminous galaxies at high-redshift are the most luminous, heavily star-forming galaxies in the Universe, and are characterised by prodigious emission in the far-infra…
What shapes the far-infrared spectral energy distributions of galaxies?
Mohammadtaher Safarzadeh, Christopher C. Hayward, Henry C. Ferguson +1
To explore the connection between the global physical properties of galaxies and their far-infrared (FIR) spectral energy distributions (SEDs), we study the variation in the FIR SE…
Deriving star formation histories from photometry using energy balance spectral energy distribution modelling
Daniel J. B. Smith, Christopher C. Hayward
Panchromatic spectral energy distribution (SED) fitting is a critical tool for determining the physical properties of distant galaxies, such as their stellar mass and star formatio…