How to distinguish a nearly flat Universe from a flat Universe using the orientation independence of a comoving standard ruler

B. F. Roukema

doi:10.1051/0004-6361:20010174

Free Access

Issue		A&A Volume 369, Number 3, April III 2001


Page(s)		729 - 735
Section		Astrophysical processes
DOI		https://doi.org/10.1051/0004-6361:20010174
Published online		15 April 2001

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