An Overview of Uncovered and Suspected Large-Scale Structures behind the Milky Way
Renée C. Kraan-Korteweg , Patrick A. Woudt, PASA, 16 (1), 53
The html and gzipped postscript versions of this paper are in preprint form.
To access the final published version, download the pdf file.
An Overview of Uncovered and Suspected Large-Scale Structures behind the Milky Way
Renée C. Kraan-Korteweg 1
Patrick A. Woudt 2
1 Depto. de Astronomía, Univ. de Guanajuato, Apartado
Postal 144, Guanajuato GTO 36000, Mexico
kraan@astro.ugto.mx
2 ESO, Karl-Schwarzschildstr. 2, D-85748 Garching bei München,
Germany
pwoudt@eso.org
Abstract:
Various dynamically important extragalactic large-scale structures
in the local Universe lie behind the Milky Way.
Most of these structures (predicted and unexpected) have only
recently been made ``visible'' through dedicated deep
surveys at various wavelengths. The wide range of
observational searches (optical, near infrared, far infrared, radio and X-ray)
for galaxies in the Zone of Avoidance (ZOA)
will be reviewed and the uncovered
and suspected large-scale structures summarised. Particular emphasis
is given to the Great Attractor region where the existence of yet
another cluster is suspected (Woudt 1998). Predictions from
reconstructions of the density field in the ZOA
are discussed and compared with observational evidence. Although
no major structures are predicted out to about

kms
-1 for which no observational evidence exists, the comparison between
reconstructed density fields and the observed galaxy distribution
remain important as they allow derivations of the density and
biasing parameters.
Keywords:
zone of avoidance --
surveys -- ISM: dust, extinction --
large-scale structure of universe
|
© Copyright Astronomical Society of Australia 1997