The Araucaria Project: The Local Group Galaxy WLM-Distance and Metallicity from Quantitative Spectroscopy of Blue Supergiants

Astrophysical Journal

dc.creatorUrbaneja, M.
dc.creatorGieren, W.
dc.creatorPietrzynski, G.
dc.date2020-03-11T20:26:29Z
dc.date2022-07-07T23:44:05Z
dc.date2020-03-11T20:26:29Z
dc.date2022-07-07T23:44:05Z
dc.date2008
dc.date.accessioned2023-08-23T00:18:45Z
dc.date.available2023-08-23T00:18:45Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/238027
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8354640
dc.descriptionThe quantitative analysis of low resolution spectra of A and B supergiants is used to determine a distance modulus of 24.99 +/- 0.10 mag (995 +/- 46 Kpc) to the Local Group galaxy WLM. The analysis yields stellar effective temperatures and gravities, whic
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationhttps://doi.org/10.1086/590334
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleThe Araucaria Project: The Local Group Galaxy WLM-Distance and Metallicity from Quantitative Spectroscopy of Blue Supergiants
dc.titleAstrophysical Journal
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


Este ítem pertenece a la siguiente institución