NDLI: SPH simulations of star/planet formation triggered by cloud-cloud collisions

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SPH simulations of star/planet formation triggered by cloud-cloud collisions

Content Provider	Scilit
Author	Kitsionas, Spyridon Whitworth, Anthony P. Klessen, Ralf S.
Copyright Year	2007
Description	We 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.
Related Links	https://www.cambridge.org/core/services/aop-cambridge-core/content/view/F0745557E56EC52AADC7AD21958A62B7/S1743921308016694a.pdf/div-class-title-sph-simulations-of-star-planet-formation-triggered-by-cloud-cloud-collisions-div.pdf
Ending Page	278
Page Count	8
Starting Page	271
ISSN	17439213
e-ISSN	17439221
DOI	10.1017/s1743921308016694
Journal	Proceedings of the International Astronomical Union
Issue Number	S249
Volume Number	3
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	2007-10-01
Access Restriction	Open
Subject Keyword	Proceedings of the International Astronomical Union Astronomy and Astrophysics Numerical Protoplanetary Disks Formation
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics Space and Planetary Science

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