| dc.contributor.author |
Vranješ, D. |
|
| dc.contributor.author |
Smiljić, Dj. |
|
| dc.contributor.author |
Gligorić, M. |
|
| dc.contributor.author |
Rakić, N. |
|
| dc.contributor.author |
Obradović, D. |
|
| dc.contributor.author |
Kovačević, J. |
|
| dc.contributor.editor |
Kovačević, Andjelka |
|
| dc.date.accessioned |
2011-01-25T10:17:32Z |
|
| dc.date.available |
2011-01-25T10:17:32Z |
|
| dc.date.issued |
2008 |
|
| dc.identifier.isbn |
978-86-80019-30-7 |
en_US |
| dc.identifier.uri |
http://hdl.handle.net/123456789/1558 |
|
| dc.description.provenance |
Submitted by Slavisha Milisavljevic (slavisha) on 2011-01-25T10:17:32Z
No. of bitstreams: 1
Vranjes.pdf: 783135 bytes, checksum: 158c8f18a82c238495bba3e47bc97fdb (MD5) |
en |
| dc.description.provenance |
Made available in DSpace on 2011-01-25T10:17:32Z (GMT). No. of bitstreams: 1
Vranjes.pdf: 783135 bytes, checksum: 158c8f18a82c238495bba3e47bc97fdb (MD5)
Previous issue date: 2008 |
en |
| dc.language.iso |
en |
en_US |
| dc.publisher |
Astronomical Observatory Belgrade |
en_US |
| dc.title |
The flux ratio of the [OIII] λλ5007, 4959 Ǻ lines in AGN |
en_US |
| dc.title.alternative |
~ analysis of the sample with red asymmetry and without asymmetry of [OIII] line profiles ~ |
en_US |
| mf.subject.area |
9 |
en_US |
| mf.subject.keywords |
Here we present the measurements of the flux ratio of the [OIII] λλ4959, 5007 Ǻ
emission lines for the sample of 10 AGNs, obtained from SDSS Database and from the published
observations. We selected the sample using the criteria of high signal to noise ratio and the same
line shapes of λ4959 and λ5007 lines. We separated our sample in two subsamples: first one with
red asymmetry of [OIII] λλ4959, 5007 Ǻ lines, where we obtained the average flux ratio of 2.981 ±
0.268 and second one with no asymmetry of [OIII] λλ4959, 5007 Ǻ lines, where we obtained the
average flux ratio of 2.885 ± 0.173. For the total sample of ten spectra we found that the flux ratio
is 2.943 ± 0.149 so the theoretical value of 2.98 befalls within the error band of our result. |
en_US |
| mf.document.pages |
9 |
en_US |
| mf.contributor.editor-in-chief |
Dimitrijević, S. Milan |
|
| mf.contributor.technical-editor |
Milovanov, Tatjana |
|