EVOLUTION OF A 30 SOLAR MASS, POPULATION I STAR,

Abstract

The problem of stellar evolution can be divided into three phases: the formation of stars from the interstellar medium; the evolution of stars through various stages of expansion and contraction, increasing and decreasing brightness and temperature, and through various changes in chemical constituents, the question of the final stellar state. In this thesis the second phase of the problem is investigated for a 30 solar mass star of Population I.

Document Details

Document Type
Technical Report
Publication Date
Jul 01, 1968
Accession Number
AD0674630

Entities

People

  • Alan M. Schindler

Organizations

  • Brandeis University

Tags

DTIC Thesaurus Topics

  • Application Software
  • Astronomy
  • Brightness
  • Computer Programs
  • Digital Information
  • Evolution (Development)
  • Evolution (General)
  • Interdisciplinary Science
  • Personal Information Managers
  • Stellar Evolution

Fields of Study

  • Physics

Readers

  • Astronomy/Astrophysics
  • Materials Science and Engineering.
  • Space Exploration and Orbital Mechanics.

Technology Areas

  • Space
  • Space - Hall-Effect Thruster
  • Space - Spacecraft Maneuvers