The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151
Autor: | Bradley M. Peterson, E. Dalla Bontà, Laura Ferrarese, Christopher A. Onken, S. L. Hoffmann, Wenlong Yuan, J. S. Brown, Lucas M. Macri, Ric Davies, E. K. S. Hicks, G. De Rosa, C. J. Grier, Marianne Vestergaard, Thaisa Storchi-Bergmann, Richard W. Pogge, Misty C. Bentz, Adam G. Riess, Michael Fausnaugh |
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Rok vydání: | 2020 |
Předmět: |
Cepheid variable stars
ACTIVE GALACTIC NUCLEI Cepheid variable Astrophysics::High Energy Astrophysical Phenomena Near infrared astronomy Galaxy distances FOS: Physical sciences Time series analysis Distance indicators REVERBERATION MAPPING DATA MAGNITUDES Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics MASS GRAVITATIONAL LENSING EXPERIMENT SUPERMASSIVE BLACK-HOLES Hubble space telescope Hubble Space Telescope Astrophysics::Solar and Stellar Astrophysics HST photometry KINEMATICS OGLE-III CATALOG Solar and Stellar Astrophysics (astro-ph.SR) Astrophysics::Galaxy Astrophysics AGN host galaxies Physics Astronomy and Astrophysics Astrophysics - Astrophysics of Galaxies Galaxy NARROW-LINE REGION Cepheid distance Astrophysics - Solar and Stellar Astrophysics GEMINI NIFS Distance measure Optical observatories Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) |
Zdroj: | Yuan, W, Fausnaugh, M M, Hoffmann, S L, Macri, L M, Peterson, B M, Riess, A G, Bentz, M C, Brown, J S, Dalla Bonta, E, Davies, R, De Rosa, G, Ferrarese, L, Grier, C J, 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, vol. 902, no. 1, 26 . https://doi.org/10.3847/1538-4357/abb377 |
ISSN: | 1538-4357 0004-637X |
DOI: | 10.3847/1538-4357/abb377 |
Popis: | We derive a distance of $15.8\pm0.4$ Mpc to the archetypical 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 ($P > 25$d) 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. 18 pages. 11 figures. 7 tables. Accepted for publication in ApJ |
Databáze: | OpenAIRE |
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