Discovery of soft and hard X-ray time lags in low-mass AGNs
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Cita com:
hdl:2117/360207
Tipus de documentArticle
Data publicació2021-03-05
EditorOxford University Press
Condicions d'accésAccés obert
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Reconeixement-NoComercial-SenseObraDerivada 3.0 Espanya
Abstract
The scaling relations between the black hole (BH) mass and soft lag properties for both active galactic nuclei (AGNs) and BH X-ray binaries (BHXRBs) suggest the same underlying physical mechanism at work in accreting BH systems spanning a broad range of mass. However, the low-mass end of AGNs has never been explored in detail. In this work, we extend the existing scaling relations to lower mass AGNs, which serve as anchors between the normal-mass AGNs and BHXRBs. For this purpose, we construct a sample of low-mass AGNs (¿MBH<3×106M¿¿) from the XMM–Newton archive and measure frequency-resolved time-delays between the soft (0.3–1 keV) and hard (1–4 keV) X-ray emissions. We report that the soft band lags behind the hard band emission at high frequencies ~[1.3-2.6] × 10-3 Hz, which is interpreted as a sign of reverberation from the inner accretion disc in response to the direct coronal emission. At low frequencies (~[3-8] × 10-4 Hz), the hard-band lags behind the soft-band variations, which we explain in the context of the inward propagation of luminosity fluctuations through the corona. Assuming a lamppost geometry for the corona, we find that the X-ray source of the sample extends at an average height and radius of ~10rg and ~6rg, respectively. Our results confirm that the scaling relations between the BH mass and soft lag amplitude/frequency derived for higher mass AGNs can safely extrapolate to lower mass AGNs, and the accretion process is indeed independent of the BH mass.
CitacióMallick, L. [et al.]. Discovery of soft and hard X-ray time lags in low-mass AGNs. "Monthly notices of the Royal Astronomical Society", 5 Març 2021, vol. 503, núm. 3, p. 3775-3783.
ISSN1365-2966
Versió de l'editorhttps://academic.oup.com/mnras/article-abstract/503/3/3775/6159464
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