Deuterium burning in objects forming via the core accretion scenario

Author: Mollière P.   Mordasini C.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|547|issue|A105-A105

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.547, Iss.issue, 2012-11, pp. : A105-A105

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Aims. Our aim is to study deuterium burning in objects forming according to the core accretion scenario in the hot and cold start assumption and what minimum deuterium burning mass limit is found for these objects. We also study how the burning process influences the structure and luminosity of the objects. Furthermore we want to test and verify our results by comparing them to already existing hot start simulations which did not consider, however, the formation process.