( en | de | ru )

 

Disambiguation of "Hayward, Christopher C."

Author of the publication

copydeleteadd this publication to your clipboard
Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo

, , , , , , , , , , , , , , , , , , , , , , and . (2022)cite arxiv:2203.14972Comment: Accepted for publication in ApJ Letters, 9 pages, 5 figures. Interactive versions of Fig. 2 and data products are available at https://github.com/spt-smg/publicdata.

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed. You can also use the button next to the name to display some publications already assigned to the person.

Christopher C Strelioff

Peter Hayward

Sandra Scott-Hayward

Christopher Christopher

Guido C C Clinckspoor

 

Other publications of authors with the same name

Predictions of the LCII -- SFR and CII Luminosity Function at the Epoch of Reionization, , , , , , , and . (2020)cite arxiv:2004.11912Comment: 17 pages, 13 figures, submitted to the ApJ.Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations, , , , , , , , , and . (2022)cite arxiv:2203.06201Comment: 18 pages, 9 figures. Submitted to MNRAS, comments welcome.Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions, , , , , , , and . (2019)cite arxiv:1912.04290Comment: submitted to MNRAS-Letters.Feedback first: the surprisingly weak effects of magnetic fields, viscosity, conduction, and metal diffusion on galaxy formation, , , , , , and . (Jul 18, 2016)Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?, , and . (2017)cite arxiv:1705.05377Comment: 6 pages, 3 figures, submitted to ApJL.The total infrared luminosity may significantly overestimate the star formation rate of recently quenched galaxies, , , , , , , , , and . (2014)cite arxiv:1402.0006Comment: 6 pages, 3 figures. Submitted to MNRAS Letters. Comments encouraged.Galaxy mergers on a moving mesh: a comparison with smoothed-particle hydrodynamics, , , , and . (2013)cite arxiv:1309.2942Comment: Submitted to MNRAS. Animations for all simulations available at http://www.cfa.harvard.edu/itc/research/arepomerger/ . 25 pages, 14 figures. Comments encouraged.How stellar feedback simultaneously regulates star formation and drives outflows, and . (2015)cite arxiv:1510.05650Comment: Fig. 5 illustrates the key conclusion. Submitted to MNRAS. Comments welcome.Star(bursts) of FIRE: observational signatures of bursty star formation in galaxies, , , , , , and . (2015)cite arxiv:1510.03869Comment: 21 pages, 15 figures, submitted to MNRAS.FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation, , , , , , , , , and 18 other author(s). (2017)cite arxiv:1702.06148Comment: 66 pages, 39 figures. Simulation animations and visualizations available at http://www.tapir.caltech.edu/~phopkins/Site/animations and http://fire.northwestern.edu Paper includes complete FIRE algorithms and public ICs (http://www.tapir.caltech.edu/~phopkins/publicICs).