A QSO survey via optical variability and zero proper motion in the M92 field.III. Narrow emission line galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10 pages, 8 figures, accepted for publication in Astronomy & Astrophysics

Scientific paper

10.1051/0004-6361:20020797

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 HII region-like spectra. No AGN could be proved, yet we cannot rule out the existence of faint low-luminosity AGNs masked by HII regions from intense star formation.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

A QSO survey via optical variability and zero proper motion in the M92 field.III. Narrow emission line galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A QSO survey via optical variability and zero proper motion in the M92 field.III. Narrow emission line galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A QSO survey via optical variability and zero proper motion in the M92 field.III. Narrow emission line galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-496869

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.