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The cepheid distance to the seyfert 1 galaxy NGC 4151

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dc.contributor.authorYuan, W
dc.contributor.authorFausnaugh, M.M.
dc.contributor.authorHoffman, Stephen L
dc.contributor.authorMacri, Lucas M.
dc.contributor.authorPeterson, Bradley M
dc.contributor.authorRiess, A G
dc.contributor.authorBentz, M C
dc.contributor.authorBrown, J. S.
dc.contributor.authorDalla Bonta, E
dc.contributor.authorDavies, Richard I
dc.contributor.authorOnken, Christopher
dc.date.accessioned2022-07-22T01:53:00Z
dc.date.available2022-07-22T01:53:00Z
dc.date.issued2020
dc.date.updated2021-08-01T08:23:30Z
dc.description.abstractWe 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.en_AU
dc.description.sponsorshipSupport for HST program GO-13765 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. MV gratefully acknowledges support from the Independent Research Fund Denmark via grant number DFF 8021-00130.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-637Xen_AU
dc.identifier.urihttp://hdl.handle.net/1885/269873
dc.language.isoen_AUen_AU
dc.provenancehttps://v2.sherpa.ac.uk/id/publication/6401..."The Published Version can be archived in any website" from SHERPA/RoMEO site (as at 22/07/2022).en_AU
dc.publisherThe American Astronomical Societyen_AU
dc.rights© 2020. The American Astronomical Societyen_AU
dc.sourceThe Astrophysical Journalen_AU
dc.subjectCepheid variable starsen_AU
dc.subjectDistance measureen_AU
dc.subjectCepheid distanceen_AU
dc.subjectAGN host galaxiesen_AU
dc.subjectHubble Space Telescopeen_AU
dc.subjectHST photometryen_AU
dc.subjectTime series analysisen_AU
dc.subjectNear infrared astronomyen_AU
dc.subjectOptical observatoriesen_AU
dc.subjectDistance indicatorsen_AU
dc.subjectGalaxy distancesen_AU
dc.titleThe cepheid distance to the seyfert 1 galaxy NGC 4151en_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1en_AU
local.bibliographicCitation.lastpage15en_AU
local.bibliographicCitation.startpage1en_AU
local.contributor.affiliationYuan, W, Johns Hopkins Universityen_AU
local.contributor.affiliationFausnaugh, M.M., Department of Astronomyen_AU
local.contributor.affiliationHoffman, Stephen L, Sanaria Inc.en_AU
local.contributor.affiliationMacri, Lucas M., Texas A&M Universityen_AU
local.contributor.affiliationPeterson, Bradley M, Ohio State Universityen_AU
local.contributor.affiliationRiess, A G, Johns Hopkins Universityen_AU
local.contributor.affiliationBentz, M C, University of Californiaen_AU
local.contributor.affiliationBrown, J. S., University of Californiaen_AU
local.contributor.affiliationDalla Bonta, E, Universita degli Studi di Padovaen_AU
local.contributor.affiliationDavies, Richard I, Max Planck Institute for Extraterrestrial Physicsen_AU
local.contributor.affiliationOnken, Christopher, College of Science, ANUen_AU
local.contributor.authoruidOnken, Christopher, u4606113en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor000000 - Internal ANU use onlyen_AU
local.identifier.ariespublicationa383154xPUB14513en_AU
local.identifier.citationvolume902en_AU
local.identifier.doi10.3847/1538-4357/abb377en_AU
local.identifier.scopusID2-s2.0-85092671134
local.publisher.urlhttp://iopscience.iop.org/0004-637Xen_AU
local.type.statusPublished Versionen_AU

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