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.

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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Status:	Unpublished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:	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

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