The Cepheid Distance to the Narrow-Line Seyfert 1 Galaxy NGC 4051

Abstract

We derive a distance of $D=16.6\pm 0.3$~Mpc ($\mu =31.10\pm 0.04$~mag) to the archetypal narrow-line Seyfert 1 galaxy NGC 4051 based on Cepheid Period--Luminosity relations and new Hubble Space Telescope multiband imaging. We identify 419 Cepheid candidates and estimate the distance at both optical and near-infrared wavelengths using subsamples of precisely-photometered variables (123 and 47 in the optical and near-infrared subsamples, respectively). We compare our independent photometric procedures and distance-estimation methods to those used by the SH0ES team and find agreement to 0.01~mag. The distance we obtain suggests an Eddington ratio $\dot{m}\approx 0.2$ for NGC 4051, typical of narrow-line Seyfert 1 galaxies, unlike the seemingly-odd value implied by previous distance estimates. We derive a peculiar velocity of $-490\pm 34$~km~s${}^{-1}$ for NGC 4051, consistent with the overall motion of the Ursa Major Cluster in which it resides. We also revisit the energetics of the NGC 4051 nucleus, including its outflow and mass accretion rates.

15 pages, 12 figures, 6 tables, accepted for publication in ApJ

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Cited by in corpus (8)

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• Cosmicflows-4
• The AGNIFS survey: spatially resolved observations of hot molecular and ionised outflows in nearby active galaxies
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• Investigating the Narrow Line Region Dynamics in Nearby Active Galaxies
• Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN
• Constraints on the ultra-fast outflows in the narrow-line Seyfert 1 galaxy Mrk 1044 from high-resolution time- and flux-resolved spectroscopy
• Detection of X-ray/UV delay in NGC 4051 using AstroSat observations