Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-48291
Commerçon, B; Hennebelle, P; Audit, E; Chabrier, G; Teyssier, R (2010). Radiative, magnetic and numerical feedbacks on small-scale fragmentation. Proceedings of the International Astronomical Union, 6(S270):227-230.
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Radiative feedback and magnetic field are understood to have a strong impact on the protostellar collapse. We present high resolution numerical calculations of the collapse of a 1 Msolar dense core in solid body rotation, including both radiative transfer and magnetic field. Using typical parameters for low-mass cores, we study thoroughly the effect of radiative transfer and magnetic field on the first core formation and fragmentation. We show that including the two aforementioned physical processes does not correspond to the simple picture of adding them separately. The interplay between the two is extremely strong, via the magnetic braking and the radiation from the accretion shock.
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|Item Type:||Journal Article, not refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Dewey Decimal Classification:||530 Physics|
|Deposited On:||19 Feb 2012 20:03|
|Last Modified:||05 Apr 2016 14:55|
|Publisher:||Cambridge University Press|
|ISSN:||1743-9213 (P) 1743-9221 (E)|
|Additional Information:||Published online: 27 April 2011. - Copyright: Cambridge University Press. - Proceedings of IAU Symposium 270: Computational Star Formation, May 31-June 4, 2010, Barcelona, Spain|
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