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20082025
most citedSpectral Optical Monitoring of the Narrow Line Seyfert 1 galaxy Ark 564

100 citations · 677 across the 52 of their papers we have counts for

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Showing 2012Show all

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astro-ph.CO2012★ 100 cited

Spectral Optical Monitoring of the Narrow Line Seyfert 1 galaxy Ark 564

A. I. Shapovalova, L. C. Popovic, A. N. Burenkov +14

We present the results of a long-term (1999--2010) spectral optical monitoring campaign of the active galactic nucleus (AGN) Ark 564, which shows a strong Fe II line emission in th…

astro-ph.SR2012★ 2 cited

Stark Broadening of in III Lines in Astrophysical and Laboratory Plasma

Z. Simic, M. S. Dimitrijevic, A. B. Kovacevic +1

Besides the need of Stark broadening parameters for a number of problems in physics, and plasma technology, in hot star atmospheres the conditions exist where Stark widths are comp…

astro-ph.SR2012★ 1 cited

Stark Broadening and White Dwarfs

Milan S. Dimitrijevic, Andjelka Kovacevic, Zoran Simic +1

White dwarf and pre-white dwarf atmospheres are one of the best examples for the application of Stark broadening research results in astrophysics, due to plasma conditions very fav…

astro-ph.SR2012★ 4 cited

Stark Broadening of several Ar I Spectral Lines in the Visible Part of the Spectrum

Milan S. Dimitrijevic, Andjelka Kovacevic, Zoran Simic +1

In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we determined Stark widths and shifts due to electron, proton, and ionized helium im…

astro-ph.SR2012★ 3 cited

Stark Broadening of several Ne II, Ne III and O III Spectral Lines for the Stark-B Database

Milan S. Dimitrijevic, Andjelka Kovacevic, Zoran Simic +1

In order to complete Stark broadening data for Ne II, and O III lines, needed for analysis of stellar atmospheres, we determined, within the semiclassical perturbation method, the…

astro-ph.CO2012★ 2 cited

Spectral monitoring of AGNs: Preliminary results for Ark 564 and Arp 102B

A. I. Shapovalova, L. C. Popovic, D. Ilic +4

We present preliminary results of the long term spectral monitoring of two active galactic nuclei with different broad line shapes: Ark 564 and Arp 102B. Ark 564 is a bright nearby…