Multiple star formation in isolated cores

Goodwin, Simon, Whitworth, Anthony Peter ORCID: https://orcid.org/0000-0002-1178-5486 and Ward-Thompson, Derek ORCID: https://orcid.org/0000-0003-1140-2761 2003. Multiple star formation in isolated cores. Presented at: International Astronomical Union Symposium 221, Sydney, Australia, 22-25 July 2003.

Full text not available from this repository.

Abstract

We present the results of over 100 simulations of star formation in turbulent molecular cores. Moderate levels of turbulence very often form several stars and brown dwarfs. Most often a central binary star forms with two unequal components in highly elliptical orbits. Smaller objects are dynamically ejected truncating their growth and creating a high-velocity low-mass population

Item Type:	Conference or Workshop Item (Poster)
Date Type:	Completion
Status:	Unpublished
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Last Modified:	27 Oct 2022 10:03
URI:	https://orca.cardiff.ac.uk/id/eprint/68777

Actions (repository staff only)

Edit Item