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Table · dataset · 2022

Lijiang/YFOSC light curves of NGC 2617

Listed in IVOA Registry (Virtual Observatory)

NGC 2617 attracted a lot of attention after the detection of changes in its spectral type; the geometry and kinematics of the broad-line region (BLR) are still ambiguous.

Description

In this paper, we present the high cadence (~2 days) reverberation mapping campaign of NGC 2617 from 2019-October to 2020-May undertaken at the Lijiang 2.4m telescope. For the first time, the velocity-resolved reverberation signature of the object was successfully detected.

Both H{alpha} and H{beta} show an asymmetrical profile with a peak in the velocity-resolved time lags. For both of the lines, the lag of the line core is longer than those of the relevant wings, and the peak of the velocity-resolved lags is slightly blueshifted. These characteristics are not consistent with the theoretical prediction of the inflow, outflow or Keplerian disk model.

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Our observations give the time lags of H{alpha}, H{beta}, H{gamma}, and HeI, with a ratio of {tau}_H{alpha}_:{tau}_H{beta}_: {tau}_H{gamma}_:{tau}_HeI_=1.27:1.00:0.89:0.20, which indicates a stratified structure in the BLR of the object. It is the first time that the lags of H{alpha} and HeI are obtained. Assuming a virial factor of f=5.5 for the dispersion width of the line, the masses of the black holes derived from H{alpha} and H{beta} are 23.8_-2.7_^+5.4^ and 21.1_-4.4_^+3.8^x10^6^M_{sun}_, respectively.

Our observed results indicate the complexity of the BLR of NGC 2617.

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