Kinematics suggest large masses for high redshift galaxies
Year: 2025
Type: other
Abstract: This is what I hope will be the final installment in a series of posts describing the results published in McGaugh et al. (2024). I started by discussing the timescale for galaxy formation in LCDM and MOND which leads to different and distinct predictions.
DOI: 10.59350/xnz7x-k7f08
Author: Stacy McGaugh
Institution: Case Western Reserve University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
OpenAlex ID: W4414859083
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