<p>This thesis reports the results of a twofold study on the recently proposed phenomenon of &lsquo / stellar pulsations&rsquo / in young brown dwarfs by the seminal study of Palla and Baraffe (2005) (PB05, thereafter). The PB05 study presents results of a non-adiabatic linear stability analysis showing that young brown dwarfs should become pulsationally unstable during the deuterium burning phase of their evolution.</p>
Identifer | oai:union.ndltd.org:UNWC/oai:UWC_ETD:http%3A%2F%2Fetd.uwc.ac.za%2Findex.php%3Fmodule%3Detd%26action%3Dviewtitle%26id%3Dgen8Srv25Nme4_4946_1308548503 |
Date | January 2011 |
Creators | Okeng'o, Geoffrey Onchongâa |
Source Sets | Univ. of Western Cape |
Language | English |
Detected Language | English |
Type | Thesis and dissertation |
Format | |
Coverage | ZA |
Rights | Copyright: University of the Western Cape |
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