The backreaction of stellar wobbling on accretion discs of massive protostars

Open Access

Table 1

Simulation models performed in our study.

Models	M_c (M_⊙)	Grid resolution	β (%)	t_end (kyr)	Wobbling
Run–512–100 M_⊙−4%-wio	100	512 × 81 × 512	4	32.65	No
Run–512–100 M_⊙−4%-wi	100	512 × 81 × 512	4	32.65	Yes

Notes. The table provides the initial mass of the molecular pre-stellar core M_c (in M_⊙), its initial rotational-to-gravitational energy ratio β (in %), and the final simulation time t_end in each model. The last column indicates whether the simulation includes stellar wobbling or not.

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