Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-27T00:27:01.206Z Has data issue: false hasContentIssue false

Properties of the Low-z NELGs from the VPM Survey

Published online by Cambridge University Press:  12 April 2016

Helmut Meusinger
Affiliation:
Thüringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany
Jens Brunzendorf
Affiliation:
Thüringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany

Abstract

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.

We discuss the properties of the low-redshift narrow-emission line galaxies detected in the framework of a variability-and-proper motion (VPM) search for AGNs. The VPM-NELG sample is obviously not a random selection of normal field galaxies.

Type
Part 1. Optical Surveys for AGN
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Ho, L.C., Filippenko, A.V., & Sargent, W.L.W. 1997, ApJ, 487, 568 Google Scholar
Meusinger, H., & Brunzendorf, J. 2001, A&A, 374, 878 Google Scholar
Osterbrock, D.E. 1989, Astrophysics of Gaseous Nebulae and Active Galactic Nuclei, Univ. Sci. Books, Mill Valley CrossRefGoogle Scholar
Sarajedini, V.L., Green, R.F., Griffiths, R.E. et al. 1999, ApJ, 524, 746 Google Scholar