Quasi-static evolution of a two component galaxy model is taken into account. The aim is to find a relationship between the tidal radius, induced by the dark matter component on the bright one, and the angular momentum in the two limit cases of late-type and early -type galaxies.

Relationship between tidal radius and angular momentum in a two component disk-galaxy system

SECCO, LUIGI ENRICO
2001

Abstract

Quasi-static evolution of a two component galaxy model is taken into account. The aim is to find a relationship between the tidal radius, induced by the dark matter component on the bright one, and the angular momentum in the two limit cases of late-type and early -type galaxies.
2001
Galaxy Disks and Disk Galaxies
1583810633
File in questo prodotto:
Non ci sono file associati a questo prodotto.
Pubblicazioni consigliate

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/1367145
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? ND
social impact