Accelerating infall and rotational spin-up in the hot molecular core G31.41+0.31
M. T. Beltr\'an (1), R. Cesaroni (1), V.M. Rivilla (1), \'A., S\'anchez-Monge (2), L. Moscadelli (1), A. Ahmadi (3), V. Allen (4, 5), H., Beuther (3), S. Etoka (6), D. Galli (1), R. Galv\'an-Madrid (7), C. Goddi (8,, 9), K.G. Johnston (11), A. K\"olligan (12), R. Kuiper (12)

TL;DR
This study uses high-resolution ALMA observations to reveal that the hot molecular core G31.41+0.31 exhibits accelerating infall and rotation, indicating gravitational collapse and potential fragmentation despite its seemingly monolithic appearance.
Contribution
It provides detailed evidence of infall and rotational spin-up in a high-mass star-forming core, highlighting the role of opacity in masking fragmentation.
Findings
Velocity gradients indicate solid-body rotation.
Infall velocity increases towards the center.
Core shows signs of gravitational collapse and potential fragmentation.
Abstract
As part of our effort to search for circumstellar disks around high-mass stellar objects, we observed the well-known core G31.41+0.31 with ALMA at 1.4 mm with an angular resolution of~0.22" (~1700 au). The dust continuum emission has been resolved into two cores namely Main and NE. The Main core, which has the stronger emission and is the more chemically rich, has a diameter of ~5300 au, and is associated with two free-free continuum sources. The Main core looks featureless and homogeneous in dust continuum emission and does not present any hint of fragmentation. Each transition of CH3CN and CH3OCHO, both ground and vibrationally excited, as well as those of CH3CN isotopologues, shows a clear velocity gradient along the NE-SW direction, with velocity linearly increasing with distance from the center, consistent with solid-body rotation. However, when comparing the velocity field of…
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