SPH simulations of star/planet formation triggered by cloud-cloud collisions
2007 ◽
Vol 3
(S249)
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pp. 271-278
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Keyword(s):
Low Mass
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AbstractWe present results of hydrodynamic simulations of star formation triggered by cloud-cloud collisions. During the early stages of star formation, low-mass objects form by gravitational instabilities in protostellar discs. A number of these low-mass objects are in the sub-stellar mass range, including a few objects of planetary mass. The disc instabilities that lead to the formation of low-mass objects in our simulations are the product of disc-disc interactions and/or interactions between the discs and their surrounding gas.
2010 ◽
Vol 6
(S270)
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pp. 503-506
Keyword(s):
2020 ◽
Vol 497
(4)
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pp. 4753-4772
Keyword(s):