0124551 - ASU-R 20000004 RIV US eng C - Conference Paper (international conference)
Palouš, Jan - Ehlerová, Soňa
How to interpret the bubble dominated ISM in the LMC?
New views of the Magellanic clouds. San Francisco: Astronomical Society of the Pacific Press, 1999 - (Chu, Y.; Suntzeff, N.; Hesser, J.; Bohlender, D.), s. 62-63. IAU Symposium., 190.
[International Astronomical Union Symposium /190./. Victoria (CA), 13.07.1998-19.07.1998]
R&D Projects: GA ČR GA205/97/0699; GA AV ČR KSK1003601
Institutional research plan: CEZ:AV0Z1003909
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

Computer simulations of expanding structures in 1D and 3D are used to discuss the observed shapes and expansion velocities of HI shells and supershells.
Permanent Link: http://hdl.handle.net/11104/0022810