13
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: not found
      • Article: not found

      The H  surface brightness-radius relation: a robust statistical distance indicator for planetary nebulae

      , ,
      Monthly Notices of the Royal Astronomical Society
      Oxford University Press (OUP)

      Read this article at

      ScienceOpenPublisher
      Bookmark
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Related collections

          Most cited references321

          • Record: found
          • Abstract: not found
          • Article: not found

          Linear regression in astronomy.

            Bookmark
            • Record: found
            • Abstract: not found
            • Article: not found

            GAIA: Composition, formation and evolution of the Galaxy

              Bookmark
              • Record: found
              • Abstract: not found
              • Article: not found

              Studies of luminous stars in nearby galaxies. I. Supergiants and O stars in the Milky Way.

                Bookmark

                Author and article information

                Journal
                Monthly Notices of the Royal Astronomical Society
                Monthly Notices of the Royal Astronomical Society
                Oxford University Press (OUP)
                0035-8711
                1365-2966
                November 11 2015
                January 11 2016
                November 18 2015
                November 18 2015
                : 455
                : 2
                : 1459-1488
                Article
                10.1093/mnras/stv1516
                de502306-c735-4df9-94dc-0307d54131ae
                © 2015
                History

                Comments

                Comment on this article