The Astrophysical Journal (Jan 2024)

AGN STORM 2. VIII. Investigating the Narrow Absorption Lines in Mrk 817 Using HST-COS Observations

  • Maryam Dehghanian,
  • Nahum Arav,
  • Gerard A. Kriss,
  • Missagh Mehdipour,
  • Doyee Byun,
  • Gwen Walker,
  • Mayank Sharma,
  • Aaron J. Barth,
  • Misty C. Bentz,
  • Benjamin D. Boizelle,
  • Michael S. Brotherton,
  • Edward M. Cackett,
  • Elena Dalla Bontà,
  • Gisella De Rosa,
  • Gary J. Ferland,
  • Carina Fian,
  • Alexei V. Filippenko,
  • Jonathan Gelbord,
  • Michael R. Goad,
  • Keith Horne,
  • Yasaman Homayouni,
  • Dragana Ilić,
  • Michael D. Joner,
  • Erin A. Kara,
  • Shai Kaspi,
  • Christopher S. Kochanek,
  • Kirk T. Korista,
  • Peter Kosec,
  • Andjelka B. Kovačević,
  • Hermine Landt,
  • Collin Lewin,
  • Ethan R. Partington,
  • Luka Č. Popović,
  • Daniel Proga,
  • Daniele Rogantini,
  • Matthew R. Siebert,
  • Thaisa Storchi-Bergmann,
  • Marianne Vestergaard,
  • Timothy. Waters,
  • Jian-Min Wang,
  • Fatima Zaidouni,
  • Ying Zu

DOI
https://doi.org/10.3847/1538-4357/ad5ff4
Journal volume & issue
Vol. 972, no. 2
p. 141

Abstract

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We observed the Seyfert 1 galaxy Mrk 817 during an intensive multiwavelength reverberation mapping campaign for 16 months. Here, we examine the behavior of narrow UV absorption lines seen in the Hubble Space Telescope/Cosmic Origins Spectrograph spectra, both during the campaign and in other epochs extending over 14 yr. We conclude that, while the narrow absorption outflow system (at −3750 km s ^−1 with FWHM = 177 km s ^−1 ) responds to the variations of the UV continuum as modified by the X-ray obscurer, its total column density (log N _H = 19.5 ${}_{-0.13}^{+0.61}$ cm ^−2 ) did not change across all epochs. The adjusted ionization parameter (scaled with respect to the variations in the hydrogen-ionizing continuum flux) is log U _H = −1.0 ${}_{-0.3}^{+0.1}$ . The outflow is located at a distance smaller than 38 pc from the central source, which implies a hydrogen density of n _H > 3000 cm ^−3 . The absorption outflow system only covers the continuum emission source and not the broad emission line region, which suggests that its transverse size is small (< 10 ^16 cm), with potential cloud geometries ranging from spherical to elongated along the line of sight.

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