FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4206642444> ?p ?o ?g. }

• W4206642444 endingPage "A130" @default.
• W4206642444 startingPage "A130" @default.
• W4206642444 abstract "We have used the sample of 577 active galactic nuclei Type 1.8-2 spectra (z < 0.25), taken from Sloan Digital Sky Survey, to trace the influence of the outflow kinematics to the profiles of different emission lines (Hbeta, [O III], Halpha, [N II], [S II]). All considered lines were fitted with two Gaussian components: one which fits the core of the line, and another which fits the wings. We gave the procedure for decomposition of Halpha+[N II] wavelength band, for the spectra where these lines overlap. The influence of the gravitational/non-gravitational kinematics to the line components is investigated by comparing the dispersions of the line components with stellar velocity dispersion. We found that wing components of all considered emission lines have pure non-gravitational kinematics, the core components are consistent with gravitational kinematics for the Halpha, [N II] and [S II] lines, while in the [O III] there is evidence for contribution from non-gravitational kinematics. We adopted the wing components as proxy of the outflow contribution and we investigated the outflow kinematics by analysing the correlations between widths and between shifts of the wing components of different lines. We found the strong correlations between shifts and between wing component widths of all considered lines, with exception of the Hbeta wing component width. These correlations indicate that outflow dynamics systemically affects all emission lines in spectrum. However, it reflects with different strength in their profiles, which is observed as different widths of the wing components. The strongest outflow signature is observed in the [O III] lines, which have the broadest wing components, weaker in Halpha and [N II], and the weakest in [S II]. These results imply that considered lines arise in different parts of an outflowing region." @default.
• W4206642444 created "2022-01-26" @default.
• W4206642444 creator A5009513108 @default.
• W4206642444 creator A5036469720 @default.
• W4206642444 creator A5080707875 @default.
• W4206642444 creator A5088440981 @default.
• W4206642444 date "2022-03-01" @default.
• W4206642444 modified "2023-10-16" @default.
• W4206642444 title "Tracing the outflow kinematics in Type 2 active galactic nuclei" @default.
• W4206642444 cites W1758974919 @default.
• W4206642444 cites W1882938068 @default.
• W4206642444 cites W1963859674 @default.
• W4206642444 cites W1965659300 @default.
• W4206642444 cites W1967876247 @default.
• W4206642444 cites W1985925156 @default.
• W4206642444 cites W1993785188 @default.
• W4206642444 cites W1998729945 @default.
• W4206642444 cites W1999883030 @default.
• W4206642444 cites W2001509540 @default.
• W4206642444 cites W2004543017 @default.
• W4206642444 cites W2016904340 @default.
• W4206642444 cites W2018164129 @default.
• W4206642444 cites W2021397202 @default.
• W4206642444 cites W2021956724 @default.
• W4206642444 cites W2022616507 @default.
• W4206642444 cites W2025621984 @default.
• W4206642444 cites W2029343094 @default.
• W4206642444 cites W2042542980 @default.
• W4206642444 cites W2053229150 @default.
• W4206642444 cites W2057181130 @default.
• W4206642444 cites W2061815116 @default.
• W4206642444 cites W2076703257 @default.
• W4206642444 cites W2088034685 @default.
• W4206642444 cites W2088581684 @default.
• W4206642444 cites W2090236411 @default.
• W4206642444 cites W2092504858 @default.
• W4206642444 cites W2103530172 @default.
• W4206642444 cites W2117307008 @default.
• W4206642444 cites W2127657174 @default.
• W4206642444 cites W2152345208 @default.
• W4206642444 cites W2154889989 @default.
• W4206642444 cites W2164231865 @default.
• W4206642444 cites W2249695201 @default.
• W4206642444 cites W2291265024 @default.
• W4206642444 cites W2510079733 @default.
• W4206642444 cites W2589553623 @default.
• W4206642444 cites W2593224863 @default.
• W4206642444 cites W2740236269 @default.
• W4206642444 cites W2769676176 @default.
• W4206642444 cites W2792905005 @default.
• W4206642444 cites W2800922733 @default.
• W4206642444 cites W2887215845 @default.
• W4206642444 cites W2918006881 @default.
• W4206642444 cites W2963155438 @default.
• W4206642444 cites W2978894859 @default.
• W4206642444 cites W3012251357 @default.
• W4206642444 cites W3035685564 @default.
• W4206642444 cites W3037641373 @default.
• W4206642444 cites W3094581029 @default.
• W4206642444 cites W3098987666 @default.
• W4206642444 cites W3099330765 @default.
• W4206642444 cites W3099644107 @default.
• W4206642444 cites W3099656572 @default.
• W4206642444 cites W3099692957 @default.
• W4206642444 cites W3100415538 @default.
• W4206642444 cites W3100981399 @default.
• W4206642444 cites W3101377002 @default.
• W4206642444 cites W3102435016 @default.
• W4206642444 cites W3102816640 @default.
• W4206642444 cites W3103859359 @default.
• W4206642444 cites W3104715349 @default.
• W4206642444 cites W3104998452 @default.
• W4206642444 cites W3105117864 @default.
• W4206642444 cites W3105580933 @default.
• W4206642444 cites W3105846100 @default.
• W4206642444 cites W3105889648 @default.
• W4206642444 cites W3106053650 @default.
• W4206642444 cites W3106121613 @default.
• W4206642444 cites W3123471366 @default.
• W4206642444 cites W3125487458 @default.
• W4206642444 cites W3125978220 @default.
• W4206642444 cites W3134013739 @default.
• W4206642444 cites W3166501910 @default.
• W4206642444 cites W4211245634 @default.
• W4206642444 doi "https://doi.org/10.1051/0004-6361/202141043" @default.
• W4206642444 hasPublicationYear "2022" @default.
• W4206642444 type Work @default.
• W4206642444 citedByCount "7" @default.
• W4206642444 countsByYear W42066424442022 @default.
• W4206642444 countsByYear W42066424442023 @default.
• W4206642444 crossrefType "journal-article" @default.
• W4206642444 hasAuthorship W4206642444A5009513108 @default.
• W4206642444 hasAuthorship W4206642444A5036469720 @default.
• W4206642444 hasAuthorship W4206642444A5080707875 @default.
• W4206642444 hasAuthorship W4206642444A5088440981 @default.
• W4206642444 hasBestOaLocation W42066424441 @default.
• W4206642444 hasConcept C121332964 @default.
• W4206642444 hasConcept C124017977 @default.

• next