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- <H1>Astrophysics, abstract<BR>
- astro-ph/9501015</H1>
- <PRE>
- From: <A HREF="mailto:hdn@newt.phys.unsw.edu.au">hdn@newt.phys.unsw.edu.au</A> (Helene Di Nella)
- Date: Fri, 6 Jan 1995 14:44:51 +1100
- </PRE>
- <H2> Structure on large scale in the Universe up to the distance of 200 Mpc</H2>
- <P>
- <B>Author(s):</B> <A HREF="/find/astro-ph/1/DI+NELLA+Helene/0/1/0/all/1/1">DI NELLA Helene</A>, <A HREF="/find/astro-ph/1/PATUREL+Georges/0/1/0/all/1/1">PATUREL Georges</A>, <A HREF="/find/astro-ph/1/Observatoire+de+Lyon/0/1/0/all/1/1">Observatoire de Lyon</A> (France)<BR>
- <B>Comments:</B> 7 pages in latex format 2 figures send separately with FIGURES<BR>
- <BLOCKQUOTE>
- The distribution of galaxies up to a distance of 200 Mpc (650 million
- light-years) is flat and shows a structure like a shell roughly centered on the
- Local Supercluster (Virgo cluster). This result clearly confirms the existence
- of the hypergalactic large scale structure noted in 1988. This is presently the
- largest structure ever seen.
- </BLOCKQUOTE>
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