Journal ArticleDOI
Structure and Evolution of the Stars
Martin Schwarzschild,C. C. Kiess +1 more
Reads0
Chats0
About:
This article is published in Physics Today.The article was published on 1958-12-01. It has received 531 citations till now. The article focuses on the topics: T Tauri star & Stellar mass loss.read more
Citations
More filters
Journal ArticleDOI
Modules for Experiments in Stellar Astrophysics (MESA)
Bill Paxton,Lars Bildsten,Aaron Dotter,Aaron Dotter,Falk Herwig,Pierre Lesaffre,Francis Timmes +6 more
TL;DR: Modules for Experiments in Stellar Astrophysics (MESA) as mentioned in this paper is a suite of open source, robust, efficient, thread-safe libraries for a wide range of applications in computational stellar astrophysics.
Journal ArticleDOI
Instability, turbulence, and enhanced transport in accretion disks
Steven A. Balbus,John F. Hawley +1 more
TL;DR: In this paper, a summary of what is now known of disk turbulence and some knotty outstanding questions (e.g., what is the physics behind nonlinear field saturation?) for which we may soon begin to develop answers.
Journal ArticleDOI
Laser Compression of Matter to Super-High Densities: Thermonuclear (CTR) Applications
TL;DR: In this article, an implosion system energized by a high energy laser was proposed to compress hydrogen to more than 10,000 times liquid density by an imploding system, which makes possible efficient thermonuclear burn of small pellets of heavy hydrogen isotopes, and makes feasible fusion power reactors using practical lasers.
Journal ArticleDOI
MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
TL;DR: The Modules for Experiments in Stellar Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project as mentioned in this paper provides a set of stellar evolutionary tracks and isochrones computed using MESA, a state-of-the-art 1D stellar evolution package.
Journal ArticleDOI
Local anisotropy in self-gravitating systems
L. Herrera,N. O. Santos +1 more
TL;DR: In this article, the authors review and discuss possible causes for the appearance of local anisotropy (principal stresses unequal) in self-gravitating systems and present its main consequences.