A QSO survey via optical variability and zero proper motion in the M 92 field

Free access article

Issue		A&A Volume 390, Number 2, August I 2002


Page(s)		439 - 448
Section		Extragalactic astronomy
DOI		http://dx.doi.org/10.1051/0004-6361:20020797

A&A 390, 439-448 (2002)
DOI: 10.1051/0004-6361:20020797

III. Narrow emission line galaxies

H. Meusinger and J. Brunzendorf

Thüringer Landessternwarte Tautenburg, 07778 Tautenburg, Germany
e-mail: meus@tls-tautenburg.de, brunz@tls-tautenburg.de

(Received 26 November 2001 / Accepted 13 May 2002)

Abstract
We study a sample of 23 narrow-emission line galaxies (NELGs) which were selected by their strong variability as QSO candidates in the framework of a variability-and-proper motion QSO survey on digitised Schmidt plates. In previous work, we have shown that variability is an efficient method to find AGNs. The variability properties of the NELGs are however significantly different from those of the QSOs. The main aim of this paper is to clarify the nature of this variability and to estimate the fraction of AGN-dominated NELGs in this sample. New photometric and spectroscopic observations are presented, along with revised data from the photographic photometry. The originally measured high variability indices could not be confirmed. The diagnostic line-ratios of the NELG spectra are consistent with $\ion{H}{ii}$ region-like spectra. No AGN could be proved, yet we cannot rule out the existence of faint low-luminosity AGNs masked by $\ion{H}{ii}$ regions from intense star formation.

Key words: galaxies: active -- galaxies: starburst -- quasars: emission lines

Offprint request: H. Meusinger, meus@tls-tautenburg.de

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