Skip to main content

COMPLEX MODELING THE CHEMO-PHOTOMETRIC EVOLUTION OF DISK GALAXY

Buy Article:

$63.00 plus tax (Refund Policy)

The chemical and photometric evolution of star forming disk galaxies is investigated. Numerical simulations of the complex gasdynamical flows are based on our own coding of the Chemo-Dynamical Smoothed Particle Hydrodynamical (CD-SPH) approach, which incorporates the effect of star formation. As a first application, the model is used to describe the chemical and photometric evolution of a disk galaxy like the Milky Way.
No Reference information available - sign in for access.
No Citation information available - sign in for access.
No Supplementary Data.
No Data/Media
No Metrics

Keywords: Galaxy evolution; Milky way; SPH; Star formation in SPH

Document Type: Research Article

Affiliations: Main Astronomical Observatory, Ukrainian National Academy of Sciences, UA-03680, Golosiiv, Kiev-121, Ukraine

Publication date: 2002-01-01

More about this publication?
  • Access Key
  • Free content
  • Partial Free content
  • New content
  • Open access content
  • Partial Open access content
  • Subscribed content
  • Partial Subscribed content
  • Free trial content
Cookie Policy
X
Cookie Policy
Ingenta Connect website makes use of cookies so as to keep track of data that you have filled in. I am Happy with this Find out more