4.6 Article

THE LICK AGN MONITORING PROJECT 2011: REVERBERATION MAPPING OF MARKARIAN 50

期刊

ASTROPHYSICAL JOURNAL LETTERS
卷 743, 期 1, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/2041-8205/743/1/L4

关键词

galaxies: active; galaxies: individual (Mrk 50); galaxies: nuclei

资金

  1. NSF [AST-1107812, 1107865, 1108665, 1108835, AST-0618209]
  2. Packard Research Fellowship
  3. Direct For Mathematical & Physical Scien [808133] Funding Source: National Science Foundation
  4. Division Of Astronomical Sciences [808133] Funding Source: National Science Foundation
  5. Division Of Astronomical Sciences
  6. Direct For Mathematical & Physical Scien [0908825, 1107865, 1108835] Funding Source: National Science Foundation
  7. Division Of Astronomical Sciences
  8. Direct For Mathematical & Physical Scien [1108665] Funding Source: National Science Foundation

向作者/读者索取更多资源

The Lick AGN Monitoring Project 2011 observing campaign was carried out over the course of 11 weeks in spring 2011. Here we present the first results from this program, a measurement of the broad-line reverberation lag in the Seyfert 1 galaxy Mrk 50. Combining our data with supplemental observations obtained prior to the start of the main observing campaign, our data set covers a total duration of 4.5 months. During this time, Mrk 50 was highly variable, exhibiting a maximum variability amplitude of a factor of similar to 4 in the U-band continuum and a factor of similar to 2 in the H beta line. Using standard cross-correlation techniques, we find that H beta and H gamma lag the V-band continuum by tau(cen) = 10.64(-0.93)(+0.82) and 8.43(-1.28)(+1.30) days, respectively, while the lag of He II lambda 4686 is unresolved. The H beta line exhibits a symmetric velocity-resolved reverberation signature with shorter lags in the high-velocity wings than in the line core, consistent with an origin in a broad-line region (BLR) dominated by orbital motion rather than infall or outflow. Assuming a virial normalization factor of f = 5.25, the virial estimate of the black hole mass is (3.2 +/- 0.5) x 10(7) M-circle dot. These observations demonstrate that Mrk 50 is among the most promising nearby active galaxies for detailed investigations of BLR structure and dynamics.

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