4.7 Article

THE STRUCTURE OF THE BROAD-LINE REGION IN ACTIVE GALACTIC NUCLEI. I. RECONSTRUCTED VELOCITY-DELAY MAPS

Journal

ASTROPHYSICAL JOURNAL
Volume 764, Issue 1, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/764/1/47

Keywords

galaxies: active; galaxies: nuclei; galaxies: Seyfert

Funding

  1. Dark Cosmology Centre
  2. Royal Society Leverhulme Trust
  3. National Science Foundation [AST-1008882]
  4. NSF
  5. NSF [AST-1004756, AST-1009756]
  6. Kitzman Fellowship
  7. Israel-Niedersachsen collaboration program
  8. Zeff Fellowship
  9. National Academy of Sciences of Ukraine
  10. Russian Foundation of Research (RFBR) [12-02-01237-a]
  11. US Civilian Research and Development for Independent States of the Former Soviet Union (CRDF) [UP1-2116, UP1-2549-CR-03]
  12. Science and Technology Facilities Council [ST/K001515/1, ST/G001987/1, ST/J001651/1] Funding Source: researchfish
  13. STFC [ST/J001651/1, ST/G001987/1, ST/K001515/1] Funding Source: UKRI
  14. Direct For Mathematical & Physical Scien
  15. Division Of Astronomical Sciences [1009756, 1008882] Funding Source: National Science Foundation

Ask authors/readers for more resources

We present velocity-resolved reverberation results for five active galactic nuclei. We recovered velocity-delay maps using the maximum entropy method for four objects: Mrk 335, Mrk 1501, 3C 120, and PG 2130+099. For the fifth, Mrk 6, we were only able to measure mean time delays in different velocity bins of the H beta emission line. The four velocity-delay maps show unique dynamical signatures for each object. For 3C 120, the Balmer lines show kinematic signatures consistent with both an inclined disk and infalling gas, but the He II lambda 4686 emission line is suggestive only of inflow. The Balmer lines in Mrk 335, Mrk 1501, and PG 2130+099 show signs of infalling gas, but the He II emission in Mrk 335 is consistent with an inclined disk. We also see tentative evidence of combined virial motion and infalling gas from the velocity-binned analysis of Mrk 6. The maps for 3C 120 and Mrk 335 are two of the most clearly defined velocity-delay maps to date. These maps constitute a large increase in the number of objects for which we have resolved velocity-delay maps and provide evidence supporting the reliability of reverberation-based black hole mass measurements.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available