SIMBAD references

2015MNRAS.449L.123M - Mon. Not. R. Astron. Soc., 449, L123-L127 (2015/May-1)

An origin of arc structures deeply embedded in dense molecular cloud cores.

MATSUMOTO T., ONISHI T., TOKUDA K. and INUTSUKA S.-I.

Abstract (from CDS):

We investigated the formation of arc-like structures in the infalling envelope around protostars, motivated by the recent Atacama Large Millimeter/Submillimeter Array (ALMA) observations of the high-density molecular cloud core, MC27/L1527F. We performed self-gravitational hydrodynamical numerical simulations with an adaptive mesh refinement code. A filamentary cloud with a 0.1 pc width fragments into cloud cores because of perturbations due to weak turbulence. The cloud core undergoes gravitational collapse to form multiple protostars, and gravitational torque from the orbiting protostars produces arc structures extending up to a 1000 au scale. As well as on a spatial extent, the velocity ranges of the arc structures, ∼ 0.5 km/s, are in agreement with the ALMA observations. We also found that circumstellar discs are often misaligned in triple system. The misalignment is caused by the tidal interaction between the protostars when they undergo close encounters because of a highly eccentric orbit of the tight binary pair.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): hydrodynamics - turbulence - stars: formation - ISM: clouds - ISM: kinematics and dynamics

Simbad objects: 11

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2019.10.18-02:18:39

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