SIMBAD references

2017ApJ...834..202G - Astrophys. J., 834, 202-202 (2017/January-2)

Oscillating filaments. I. Oscillation and geometrical fragmentation.

GRITSCHNEDER M., HEIGL S. and BURKERT A.

Abstract (from CDS):

We study the stability of filaments in equilibrium between gravity and internal as well as external pressure using the grid-based AMR code RAMSES. A homogeneous, straight cylinder below a critical line mass is marginally stable. However, if the cylinder is bent, such as with a slight sinusoidal perturbation, an otherwise stable configuration starts to oscillate, is triggered into fragmentation, and collapses. This previously unstudied behavior allows a filament to fragment at any given scale, as long as it has slight bends. We call this process "geometrical fragmentation." In our realization, the spacing between the cores matches the wavelength of the sinusoidal perturbation, whereas up to now, filaments were thought to be only fragmenting on the characteristic scale set by the mass-to-line ratio. Using first principles, we derive the oscillation period as well as the collapse timescale analytically. To enable a direct comparison with observations, we study the line-of-sight velocity for different inclinations. We show that the overall oscillation pattern can hide the infall signature of cores.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): ISM: kinematics and dynamics - ISM: structure - hydrodynamics - methods: analytical - methods: numerical - stars: formation - stars: formation

Simbad objects: 3

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