A method for reconstructing the variance of a 3D physical field from 2D observations: application to turbulence in the interstellar medium (2010)
Attributed to:
The formation and evolution of stars
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2009.16215.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2009.16215.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3