Numerical simulation of high Mach number astrophysical jets with radiative cooling

Cited 27 time in webofscience Cited 0 time in scopus
  • Hit : 150
  • Download : 0
Computational fluid dynamics simulations using the WENO-LF method are applied to high Mach number nonrelativistic astrophysical jets, including the effects of radiative cooling. Our numerical methods have allowed us to simulate astrophysical jets at much higher Mach numbers than have been attained (Mach 20) in the literature. Our simulations of the HH 1-2 astrophysical jets are at Mach 80. Simulations at high Mach numbers and with radiative cooling are essential for achieving detailed agreement with the astrophysical images.
Publisher
SPRINGER/PLENUM PUBLISHERS
Issue Date
2005
Language
English
Article Type
Article
Keywords

ESSENTIALLY NONOSCILLATORY SCHEMES; PROTOSTELLAR JETS; EFFICIENT IMPLEMENTATION; SUPERSONIC JETS; HIGH-ORDER; STABILITY; INSTABILITIES; INTERFACES; DYNAMICS

Citation

JOURNAL OF SCIENTIFIC COMPUTING, v.24, no.1, pp.597 - 612

ISSN
0885-7474
DOI
10.1007/s10915-004-4786-4
URI
http://hdl.handle.net/10203/86241
Appears in Collection
Files in This Item
There are no files associated with this item.
This item is cited by other documents in WoS
⊙ Detail Information in WoSⓡ Click to see webofscience_button
⊙ Cited 27 items in WoS Click to see citing articles in records_button

qr_code

  • mendeley

    citeulike


rss_1.0 rss_2.0 atom_1.0