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Fragmentation (Interstellar Clouds)

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Encyclopedia of Astrobiology
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Synonyms

Star formation

Definition

The dense cores that form stars through gravitational collapse are embedded in much larger and more rarefied expanses of gas. How the parent molecular cloud produces its substructure of dense cores is the problem of fragmentation. The traditional view is that the parent cloud breaks apart as it collapses in on itself. In numerical simulations, objects resembling dense cores are created in turbulent, collapsing clouds. However, there is little evidence that large clouds are indeed collapsing. If they are not, but are at least temporarily stable, then dense cores must be produced in another fashion, perhaps by the slow accretion of background gas.

Overview

The interstellar clouds that contain young stars are relatively small structures embedded within more diffuse background gas. These dense cores have sizes of about 0.1 parsec, and masses comparable to that of the Sun. The diffuse parent bodies, known as dark clouds or clumps, have sizes larger by two...

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References and Further Reading

  • Hoyle F (1953) On the fragmentation of gas clouds into galaxies and stars. Astrophys J 118:513

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  • Offner S, Klein RL, McKee CF (2008) Driven and decaying turbulence simulations of low-mass star formation: from clumps to cores to protostars. Astrophys J 686:1174

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  • Stahler SW, Palla F (1994) Chapter 12. In: The formation of stars. Wiley, Weinheim

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Correspondence to Steven Stahler .

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© 2011 Springer-Verlag Berlin Heidelberg

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Stahler, S. (2011). Fragmentation (Interstellar Clouds). In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-11274-4_598

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