IUE Spectra of Seyvert 1 Galaxy NGC 7469- BLR Characteristics of NGC 7469

From the line ratios of Si III] 1892 to C III] 1909 (Feibelman & Aller 1987), we estimated the BLR electron densities and their changes of Seyfert 1 galaxy NGC 7469 using IUE spectra observed from June 11 to July 29, 1996 (Wanders et al. 1997). We separated blended Si III] and C III] lines using...

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Main Authors: Dong-Hoon Son, Siek Hyung
Format: Article
Language:English
Published: The Korean Space Science Society 2005-09-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2005/v22n3/OJOOBS_2005_v22n3_187.pdf
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author Dong-Hoon Son
Siek Hyung
author_facet Dong-Hoon Son
Siek Hyung
author_sort Dong-Hoon Son
collection DOAJ
description From the line ratios of Si III] 1892 to C III] 1909 (Feibelman & Aller 1987), we estimated the BLR electron densities and their changes of Seyfert 1 galaxy NGC 7469 using IUE spectra observed from June 11 to July 29, 1996 (Wanders et al. 1997). We separated blended Si III] and C III] lines using the STARLINK/DIPSO and measured their fluxes within the error of 12.4% and 6.6%, respectively. Electron density fluctuated from 109.69 to 1010.93 during about two month period, i.e. 17.3 times density variation within 50 days. We also derived time delays from UV emission line variations relative to the continuum (at 1315Å): 2 days for C IV, 4 days for C III], 8 days for Si III]. This suggests that their stratified UV line emission regions are at 0.002 pc, 0.004 pc and 0.006 pc, respectively, from the central region. Based on the BLR sizes and their rotation velocities deduced from the line profiles, we estimate the central black hole mass as about 106 M⊙.
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spelling doaj.art-f98400410c3a4a57b4101fd860a3cfc12024-02-02T20:56:16ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092005-09-0122318719610.5140/JASS.2005.22.3.187IUE Spectra of Seyvert 1 Galaxy NGC 7469- BLR Characteristics of NGC 7469Dong-Hoon Son0Siek Hyung1Dept. of Astronomy and Space Science, Kyunghee UniversitySchool of Science Education (Astronomy), Chungbuk National UniversityFrom the line ratios of Si III] 1892 to C III] 1909 (Feibelman & Aller 1987), we estimated the BLR electron densities and their changes of Seyfert 1 galaxy NGC 7469 using IUE spectra observed from June 11 to July 29, 1996 (Wanders et al. 1997). We separated blended Si III] and C III] lines using the STARLINK/DIPSO and measured their fluxes within the error of 12.4% and 6.6%, respectively. Electron density fluctuated from 109.69 to 1010.93 during about two month period, i.e. 17.3 times density variation within 50 days. We also derived time delays from UV emission line variations relative to the continuum (at 1315Å): 2 days for C IV, 4 days for C III], 8 days for Si III]. This suggests that their stratified UV line emission regions are at 0.002 pc, 0.004 pc and 0.006 pc, respectively, from the central region. Based on the BLR sizes and their rotation velocities deduced from the line profiles, we estimate the central black hole mass as about 106 M⊙.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2005/v22n3/OJOOBS_2005_v22n3_187.pdfSeyfert Galaxiesactive galactic nucleiultraviolet spectra
spellingShingle Dong-Hoon Son
Siek Hyung
IUE Spectra of Seyvert 1 Galaxy NGC 7469- BLR Characteristics of NGC 7469
Journal of Astronomy and Space Sciences
Seyfert Galaxies
active galactic nuclei
ultraviolet spectra
title IUE Spectra of Seyvert 1 Galaxy NGC 7469- BLR Characteristics of NGC 7469
title_full IUE Spectra of Seyvert 1 Galaxy NGC 7469- BLR Characteristics of NGC 7469
title_fullStr IUE Spectra of Seyvert 1 Galaxy NGC 7469- BLR Characteristics of NGC 7469
title_full_unstemmed IUE Spectra of Seyvert 1 Galaxy NGC 7469- BLR Characteristics of NGC 7469
title_short IUE Spectra of Seyvert 1 Galaxy NGC 7469- BLR Characteristics of NGC 7469
title_sort iue spectra of seyvert 1 galaxy ngc 7469 blr characteristics of ngc 7469
topic Seyfert Galaxies
active galactic nuclei
ultraviolet spectra
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2005/v22n3/OJOOBS_2005_v22n3_187.pdf
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