The Pandora project - II. How non-thermal physics drives bursty star formation and temperate mass-loaded outflows in dwarf galaxies (2026)
Attributed to:
Peta-5: A National Facility for Petascale Data Intensive Computation and Analytics
funded by
EPSRC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staf2106
Publication URI: http://dx.doi.org/10.1093/mnras/staf2106
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 2