Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-03T08:30:57.786Z Has data issue: false hasContentIssue false
  • English
  • Français

Search for Emission Line Galaxies Towards nearby Voids

Published online by Cambridge University Press:  25 May 2016

C.C. Popescu ,
U. Hopp  and
H. Elsässer
C.C. Popescu
Affiliation:
Max Planck Institut f. Astronomie, D-69117 Heidelberg, FRG
U. Hopp
Affiliation:
Universitätssternwarte München, D-81679 München, FRG
H. Elsässer
Affiliation:
Max Planck Institut f. Astronomie, D-69117 Heidelberg, FRG

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Recent redshift surveys of galaxies (e.g. the Center for Astrophysics Survey (CfA)), revealed that bright galaxies are distributed in sheet-like structures which surround large voids. Still under debate is the question whether all galaxies follow such a distribution or if less luminous galaxies are more equally distributed. Given the limitation of the actual surveys, the observed emptiness of the voids may be a result of observational bias.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 434
Copyright
Copyright © Kluwer 1996