Electronic Resource
Springer
Astrophysics and space science
216 (1994), S. 311-316
ISSN:
1572-946X
Keywords:
radiative shocks
;
spectroscopy
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract This paper presents models of optical emission line features that characterise catastrophic cooling in radiative shocks. The computations are based on a 1-D magnetohydrodynamic model. Runaway cooling results in the formation of secondary shocks which travel through the previously shocked cooling layer. Several filaments of emission with specific properties and spectral signatures are produced.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00982510
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