Pittard, J.M., Arthur, S.J., Dyson, J.E., Falle, S.A.E.G., Hartquist, T.W., Knight, M.I. and Pexton, M. (2003) The evolution of mass loaded supernova remnants: II. Temperature dependent mass injection rates. Astronomy and Astrophysics, 401 (3). pp. 1027-1038. ISSN 0004-6361Full text available as:
Available under licence : See the attached licence file.
We investigate the evolution of spherically symmetric supernova remnants in which mass loading takes place due to conductively driven evaporation of embedded clouds. Numerical simulations reveal significant differences between the evolution of conductively mass loaded and the ablatively mass loaded remnants studied in Paper I. A main difference is the way in which conductive mass loading is extinguished at fairly early times, once the interior temperature of the remnant falls below ~ 107 K. Thus, at late times remnants that ablatively mass load are dominated by loaded mass and thermal energy, while those that conductively mass load are dominated by swept-up mass and kinetic energy. Simple approximations to the remnant evolution, complementary to those in Paper I, are given.
|Copyright, Publisher and Additional Information:||© ESO 2003.|
|Keywords:||kinematics, dynamics, supernova remnants,galaxies, ISM|
|Institution:||The University of Leeds|
|Academic Units:||The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds)
The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
|Depositing User:||Repository Assistant|
|Date Deposited:||02 Jun 2006|
|Last Modified:||08 Jun 2014 06:13|