[1] Ha Y, Gardner C L, Gelb A, Shu C -W. Numerical simulation of high Mach number astrophysical jets with radiative cooling. Journal of Scientific Computing, 2005, 24: 29--44
[2] Ha Y, Gardner C L. Positive scheme numerical simulation of high Mach number astrophysical jets. Journal of Scientific Computing, 2008, 34: 247--259
[3] Krist J E, Stapelfeldt K R, Burrows C J, et al. Hubble Space Telescope WFPC2 imaging of XZ Tauri: Time evolution of a Herbig-Haro bow
shock. Astrophysical Journal, 1999, 515: L35--L38
[4] Krist J E, Stapelfeldt K R, Hester J J, et al. A multi-epoch HST study of the Herbig-Haro flow from XZ Tauri. Astronomical Journal, 2008, 136: 1980--1994
[5] Schmutzler T, Tscharnuter W M. Effective radiative cooling in optically thin plasmas. Astronomy and Astrophysics, 1993, 273: 318--330
[6] Shu C -W. High order ENO and {WENO} schemes for computational fluid dynamics//High-Order Methods for Computational Physics.
Lecture Notes in Computational Science and Engineering Vol 9. New York: Springer-Verlag, 1999: 439--582
[7] Hester J J, Stapelfeldt K R, Scowen P A. Hubble space telescope wide field planetary camera 2 observations of HH 1--2. Astronomical Journal, 1998, 116: 372--395
|