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Deuterium burning in objects forming via the core accretion scenario
2012
Astronomy and Astrophysics
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. Methods. We present a
doi:10.1051/0004-6361/201219844
fatcat:2r5dbfxuuzayhnankknbzuykfu