Simulations of the grand design galaxy M51: a case study for analysing tidally induced spiral structure Simulations of tidally induced structure in M51 (2010)
Attributed to:
The formation of stars and planets: Radiation hydrodynamical and magnetohydrodynamical simulations
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2009.16161.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2009.16161.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 2