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SUMMARY:On the shape of rotating stars.
DTSTART;VALUE=DATE-TIME:20110713T131500Z
DTEND;VALUE=DATE-TIME:20110713T133000Z
DTSTAMP;VALUE=DATE-TIME:20260811T054931Z
UID:indico-contribution-5146@events.saip.org.za
DESCRIPTION:Speakers: Peter Nicol (University of Johannesburg)\nI adapt a 
 recent work by Zahn et al. on the shape of rapidly rotating stars to explo
 re the degree of oblateness for uniform\, differential and shellular rotat
 ion of the star. I also discuss the relation of these results to the class
 ical Roche limit.\n\nhttps://events.saip.org.za/event/7/contributions/5146
 /
LOCATION: Acro2
URL:https://events.saip.org.za/event/7/contributions/5146/
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