The cepheid distance to the seyfert 1 galaxy NGC 4151

W. Yuan; M. M. Fausnaugh; S. L. Hoffmann; L. M. Macri; B. M. Peterson; M. C. Bentz; J. S. Brown; E. Dalla Bontà; R. I. Davies; G. de Rosa; L. Ferrarese; C. J. Grier; A. G. Riess; E. K.S. Hicks; C. A. Onken; R. W. Pogge; T. Storchi-Bergmann; M. Vestergaard

doi:10.3847/1538-4357/abb377

The cepheid distance to the seyfert 1 galaxy NGC 4151

W. Yuan^*, M. M. Fausnaugh, S. L. Hoffmann, L. M. Macri, B. M. Peterson, M. C. Bentz, J. S. Brown, E. Dalla Bontà, R. I. Davies, G. de Rosa, L. Ferrarese, C. J. Grier, A. G. Riess, E. K.S. Hicks, C. A. Onken, R. W. Pogge, T. Storchi-Bergmann, M. Vestergaard

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

33 Citations (Scopus)

Abstract

We derive a distance of 15.8 ± 0.4 Mpc to the archetypal Seyfert 1 galaxy NGC 4151 based on the near-infrared Cepheid period–luminosity relation and new Hubble Space Telescope multiband imaging. This distance determination, based on measurements of 35 long-period (P > 25 days) Cepheids, will support the absolute calibration of the supermassive black hole mass in this system, as well as studies of the dynamics of the feedback or feeding of its active galactic nucleus.

Original language	English
Article number	26
Journal	Astrophysical Journal
Volume	902
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/abb377
Publication status	Published - 10 Oct 2020

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Yuan, W., Fausnaugh, M. M., Hoffmann, S. L., Macri, L. M., Peterson, B. M., Bentz, M. C., Brown, J. S., Dalla Bontà, E., Davies, R. I., de Rosa, G., Ferrarese, L., Grier, C. J., Riess, A. G., Hicks, E. K. S., Onken, C. A., Pogge, R. W., Storchi-Bergmann, T., & Vestergaard, M. (2020). The cepheid distance to the seyfert 1 galaxy NGC 4151. Astrophysical Journal, 902(1), Article 26. https://doi.org/10.3847/1538-4357/abb377

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title = "The cepheid distance to the seyfert 1 galaxy NGC 4151",

abstract = "We derive a distance of 15.8 ± 0.4 Mpc to the archetypal Seyfert 1 galaxy NGC 4151 based on the near-infrared Cepheid period–luminosity relation and new Hubble Space Telescope multiband imaging. This distance determination, based on measurements of 35 long-period (P > 25 days) Cepheids, will support the absolute calibration of the supermassive black hole mass in this system, as well as studies of the dynamics of the feedback or feeding of its active galactic nucleus.",

author = "W. Yuan and Fausnaugh, {M. M.} and Hoffmann, {S. L.} and Macri, {L. M.} and Peterson, {B. M.} and Bentz, {M. C.} and Brown, {J. S.} and {Dalla Bont{\`a}}, E. and Davies, {R. I.} and {de Rosa}, G. and L. Ferrarese and Grier, {C. J.} and Riess, {A. G.} and Hicks, {E. K.S.} and Onken, {C. A.} and Pogge, {R. W.} and T. Storchi-Bergmann and M. Vestergaard",

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doi = "10.3847/1538-4357/abb377",

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Yuan, W, Fausnaugh, MM, Hoffmann, SL, Macri, LM, Peterson, BM, Bentz, MC, Brown, JS, Dalla Bontà, E, Davies, RI, de Rosa, G, Ferrarese, L, Grier, CJ, Riess, AG, Hicks, EKS, Onken, CA, Pogge, RW, Storchi-Bergmann, T & Vestergaard, M 2020, 'The cepheid distance to the seyfert 1 galaxy NGC 4151', Astrophysical Journal, vol. 902, no. 1, 26. https://doi.org/10.3847/1538-4357/abb377

TY - JOUR

T1 - The cepheid distance to the seyfert 1 galaxy NGC 4151

AU - Yuan, W.

AU - Fausnaugh, M. M.

AU - Hoffmann, S. L.

AU - Macri, L. M.

AU - Peterson, B. M.

AU - Bentz, M. C.

AU - Brown, J. S.

AU - Dalla Bontà, E.

AU - Davies, R. I.

AU - de Rosa, G.

AU - Ferrarese, L.

AU - Grier, C. J.

AU - Riess, A. G.

AU - Hicks, E. K.S.

AU - Onken, C. A.

AU - Pogge, R. W.

AU - Storchi-Bergmann, T.

AU - Vestergaard, M.

PY - 2020/10/10

Y1 - 2020/10/10

N2 - We derive a distance of 15.8 ± 0.4 Mpc to the archetypal Seyfert 1 galaxy NGC 4151 based on the near-infrared Cepheid period–luminosity relation and new Hubble Space Telescope multiband imaging. This distance determination, based on measurements of 35 long-period (P > 25 days) Cepheids, will support the absolute calibration of the supermassive black hole mass in this system, as well as studies of the dynamics of the feedback or feeding of its active galactic nucleus.

AB - We derive a distance of 15.8 ± 0.4 Mpc to the archetypal Seyfert 1 galaxy NGC 4151 based on the near-infrared Cepheid period–luminosity relation and new Hubble Space Telescope multiband imaging. This distance determination, based on measurements of 35 long-period (P > 25 days) Cepheids, will support the absolute calibration of the supermassive black hole mass in this system, as well as studies of the dynamics of the feedback or feeding of its active galactic nucleus.

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U2 - 10.3847/1538-4357/abb377

DO - 10.3847/1538-4357/abb377

M3 - Article

SN - 0004-637X

VL - 902

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 26

ER -

The cepheid distance to the seyfert 1 galaxy NGC 4151

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