Hostname: page-component-6d856f89d9-jrqft Total loading time: 0 Render date: 2024-07-16T08:47:53.133Z Has data issue: false hasContentIssue false
  • English
  • Français

The Effect of Stellar Mass on Kinematical Age Determination

Published online by Cambridge University Press:  12 April 2016

Wilhelmina Iwanowska
Wilhelmina Iwanowska*
Affiliation:
Institute of Astronomy, N. Copernicus University Toruń, Poland

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

It is believed that kinematical characteristics of a group of stars, as the velocity dispersion or the lag in rotation, change systematically with time. This kinematical evolution is widely used for the determination of stellar ages. In particular, velocity dispersion should increase with time owing to irregular galactic force field. A classical formula for the increase of stellar velocity v with the age τ

Type
Part IV: Kinematics and Dynamical Evolution of the Galaxy
Information
International Astronomical Union Colloquium , Volume 45: Chemical and Dynamical Evolution of our Galaxy , September 1977 , pp. 283 - 287
Copyright
Copyright © Geneva Observatory 1977

References

Allen, C.W. : 1973, “Astrophysical Quantities”, 3rd ed.Google Scholar
Chandrasekhar, S. : 1942, “Principles of Stellar Dynamics”, University of Chicago Press Google Scholar
Iben, I. : 1967, Ann. Rev. Astron. & Astrophys. 5, 57 CrossRefGoogle Scholar
Iwanowska, W. : 1958, Bull. Astron. Obs. Toruń, No 18 Google Scholar
Lynden Bell, D. : 1967, Monthly Not. Roy. Astron. Soc. 136, 101 CrossRefGoogle Scholar
Parenago, P.P. : 1954, “Kurs zvezdnoy astronomii”, MoskvaGoogle Scholar
Spitzer, L., Schwarzschild, M. : 1953, Astrophys. J. 118, 105 CrossRefGoogle Scholar
Wielen, R. : 1974, Highlights in Astronomy, Vol. 3, 402 CrossRefGoogle Scholar