THE GALACTIC CALIBRATION OF THE CEPHEID PERIOD-LUMINOSITY RELATION AND ITS IMPLICATIONS FOR THE UNIVERSAL DISTANCE SCALE

Автор(и)

  • D. G. Turner Department of Astronomy and Physics, Saint Mary’s University, Halifax, Nova Scotia, Canada; Visiting Astronomer, Dominion Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council of Canada;, Канада
  • D. J. Majaess Department of Astronomy and Physics, Saint Mary’s University, Halifax, Nova Scotia, Canada ; The Abbey Ridge Observatory, Stillwater Lake, Nova Scotia, Canada, Канада
  • D. J. Lane Department of Astronomy and Physics, Saint Mary’s University, Halifax, Nova Scotia, Canada ; The Abbey Ridge Observatory, Stillwater Lake, Nova Scotia, Canada, Канада
  • J. M. Rosvick Thompson Rivers University, Kamloops, British Columbia, Canada; Visiting Astronomer, Dominion Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council of Canada, Канада
  • A. A. Henden AAVSO, Cambridge, Massachusetts, U.S.A., США
  • D. D. Balam Dominion Astrophysical Observatory, Victoria, British Columbia, Canada, Канада

DOI:

https://doi.org/10.18524/1810-4215.2010.23.85249

Ключові слова:

Stars, fundamental parameters, stars, variables, Cepheids, Galaxy, structure.

Анотація

The Galactic calibration of the period-luminosity (PL) relation for classical Cepheids is examined using trigonometric, open cluster, and pulsation parallaxes, which help establish independent versions of the relationship. The calibration is important for the continued use of classical Cepheids in constraining cosmological models (by refining estimates for H0), for defining zero-points for the SNe Ia and population II (Type II Cepheids/RR Lyrae variables) distance scales, for clarifying properties of the Milky Way’s spiral structure, and for characterizing dust extinction affecting Cepheids in the Milky Way and other galaxies. Described is a program to extend and refine the Galactic Cepheid PL relation by obtaining UBVRIJHKs photometry and spectra for stars in open clusters suspected of hosting classical Cepheids, using the the facilities of the OAMM, DAO, AAVSO, and ARO.

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2010-12-02

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