Kinematics suggest large masses for high redshift galaxies
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.
Authors
- Stacy McGaugh (ORCID: https://orcid.org/0000-0002-9762-0980)
Publication Details
- Journal
- Front Matter
- Published
- 2025-02-10
- DOI
- https://doi.org/10.59350/xnz7x-k7f08
- Primary Topic
- Astronomy and Astrophysical Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00