FM Vincentelli
On the multiwavelength variability of Mrk 110: two components acting at different time-scales
Vincentelli, FM; McHardy, I; Cackett, EM; Barth, AJ; Horne, K; Goad, M; Korista, K; Gelbord, J; Brandt, W; Edelson, R; Miller, JA; Pahari, M; Peterson, BM; Schmidt, T; Baldi, RD; Breedt, E; Hernández Santisteban, JV; Romero-Colmenero, E; Ward, M; Williams, DRA
Authors
I McHardy
EM Cackett
AJ Barth
K Horne
M Goad
K Korista
J Gelbord
W Brandt
R Edelson
JA Miller
M Pahari
BM Peterson
T Schmidt
RD Baldi
E Breedt
JV Hernández Santisteban
E Romero-Colmenero
Professor Martin Ward martin.ward@durham.ac.uk
Emeritus Professor
DRA Williams
Abstract
We present the first intensive continuum reverberation mapping study of the high accretion-rate Seyfert galaxy Mrk 110. The source was monitored almost daily for more than 200 d with the Swift X-ray and ultraviolet (UV)/optical telescopes, supported by ground-based observations from Las Cumbres Observatory, the Liverpool Telescope, and the Zowada Observatory, thus extending the wavelength coverage to 9100 Å. Mrk 110 was found to be significantly variable at all wavebands. Analysis of the intraband lags reveals two different behaviours, depending on the time-scale. On time-scales shorter than 10 d the lags, relative to the shortest UV waveband (∼1928 Å), increase with increasing wavelength up to a maximum of ∼2 d lag for the longest waveband (∼9100 Å), consistent with the expectation from disc reverberation. On longer time-scales, however, the g-band lags the Swift BAT hard X-rays by ∼10 d, with the z-band lagging the g-band by a similar amount, which cannot be explained in terms of simple reprocessing from the accretion disc. We interpret this result as an interplay between the emission from the accretion disc and diffuse continuum radiation from the broad-line region.
Citation
Vincentelli, F., McHardy, I., Cackett, E., Barth, A., Horne, K., Goad, M., Korista, K., Gelbord, J., Brandt, W., Edelson, R., Miller, J., Pahari, M., Peterson, B., Schmidt, T., Baldi, R., Breedt, E., Hernández Santisteban, J., Romero-Colmenero, E., Ward, M., & Williams, D. (2021). On the multiwavelength variability of Mrk 110: two components acting at different time-scales. Monthly Notices of the Royal Astronomical Society, 504(3), 4337-4353. https://doi.org/10.1093/mnras/stab1033
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 8, 2021 |
Online Publication Date | Apr 15, 2021 |
Publication Date | 2021-07 |
Deposit Date | Sep 9, 2021 |
Publicly Available Date | Sep 9, 2021 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 504 |
Issue | 3 |
Pages | 4337-4353 |
DOI | https://doi.org/10.1093/mnras/stab1033 |
Public URL | https://durham-repository.worktribe.com/output/1235176 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2021 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.https://doi.org/10.1093/mnras/stab1033
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