Star formation in X-ray cluster cooling flows

• 1 July 1987
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 318, 612-620
• https://doi.org/10.1086/165397

Abstract

Keywords

• QUANTUM MECHANICS
• STAR FORMATION
• FLOW VELOCITY
• MAGNETOHYDRODYNAMICS
• CHEMICAL COMPOSITION
• DARK MATTER
• ANALYTIC SOLUTION
• THERMAL STABILITY
• COOLING FLOW
• COSMIC RAY
• SURFACE BRIGHTNESS
• FLUID MECHANICS