The Formation of Short Period Binary Star Systems From Stable, Self-Gravitating, Gaseous Bars. | Zendy

AI Assistant Blog Pricing

Open Access

The Formation of Short Period Binary Star Systems From Stable, Self-Gravitating, Gaseous Bars.

Author(s) -

John Cazes

Publication year - 1999

Language(s) - English

Resource type - Dissertations/theses

DOI - 10.31390/gradschool_disstheses.6982

Subject(s) - physics , instability , supersonic speed , classical mechanics , oscillation (cell signaling) , mechanics , rotational symmetry , astrophysics , biology , genetics

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom

About

About Careers Publisher Partners Contact Us Get Organisational Trial or Quote

Learn

FAQs Blog Terms of Use Privacy Policy

Download the Zendy App

Download on the

Discover

Explore

Copyright Knowledge E © 2026. All Rights Reserved.