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  The Cepheid distance to the Seyfert 1 Galaxy NGC 4151

Yuan, W., Fausnaugh, M. M., Hoffmann, S. L., Macri, L. M., Peterson, B. M., Riess, A. G., et al. (2020). The Cepheid distance to the Seyfert 1 Galaxy NGC 4151. The Astrophysical Journal, 901(1): 26. doi:10.3847/1538-4357/abb377.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0007-88E3-F Version Permalink: https://hdl.handle.net/21.11116/0000-0007-88E4-E
Genre: Journal Article

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The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151.pdf (Any fulltext), 5MB
 
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 Creators:
Yuan, W., Author
Fausnaugh, M. M., Author
Hoffmann, S. L., Author
Macri, L. M., Author
Peterson, B. M., Author
Riess, A. G., Author
Bentz, M. C., Author
Brown, J. S., Author
Bontà, E. Dalla, Author
Davies, R. I.1, Author           
Rosa, G. De, Author
Ferrarese, L., Author
Grier, C. J., Author
Hicks, E. K. S., Author
Onken, C. A., Author
Pogge, R. W., Author
Storchi-Bergmann, T., Author
Vestergaard, M., Author
Affiliations:
1Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159889              

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 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.

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 Dates: 2020-10-08
 Publication Status: Published online
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 Rev. Type: -
 Identifiers: DOI: 10.3847/1538-4357/abb377
Other: LOCALID: 3270377
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Title: The Astrophysical Journal
Source Genre: Journal
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Publ. Info: Bristol; Vienna : IOP Publishing; IAEA
Pages: - Volume / Issue: 901 (1) Sequence Number: 26 Start / End Page: - Identifier: ISSN: 0004-637X
CoNE: https://pure.mpg.de/cone/journals/resource/954922828215_3