Self-similar solutions and the stability of collapsing isothermal filaments

• 1 April 1992
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 388, 392-399
• https://doi.org/10.1086/171162

Abstract

Keywords

• EARLY STARS
• GRAVITATIONAL COLLAPSE
• ISOTHERMAL PROCESSES
• STAR FORMATION
• T TAURI STARS
• EIGENVALUES
• EQUATIONS OF STATE
• NUMERICAL INTEGRATION
• PERTURBATION THEORY