HST opt. & H-band obs. of Cepheids in NGC4151 Virtual Observatory Resource

Authors
  1. Yuan W.
  2. Fausnaugh M.M.
  3. Hoffmann S.L.
  4. Macri L.M.
  5. Peterson B.M.,Riess A.G.
  6. Bentz M.C.
  7. Brown J.S.
  8. Bonta E.D.
  9. Davies R.I.
  10. De Rosa G.,Ferrarese L.
  11. Grier C.J.
  12. Hicks E.K.S.
  13. Onken C.A.
  14. Pogge R.W.,Storchi-Bergmann T.
  15. Vestergaard M.
  16. Published by
    CDS
Abstract

We derive a distance of 15.8+/-0.4Mpc 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>25d) 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.

Keywords
  1. hst-photometry
  2. visible-astronomy
  3. infrared-photometry
  4. variable-stars
  5. galaxies
Bibliographic source Bibcode
2020ApJ...902...26Y
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/902/26
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/902/26
Document Object Identifer DOI
doi:10.26093/cds/vizier.19020026

Access

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History

2022-03-08T17:28:41Z
Resource record created
2022-03-08T17:28:41Z
Created
2022-03-14T07:44:50Z
Updated

Contact

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CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
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cds-question@unistra.fr