Characteristics of the Galaxy according to Cepheids

@article{Majaess2009CharacteristicsOT,
  title={Characteristics of the Galaxy according to Cepheids},
  author={D. Majaess and D. Turner and D. Lane},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2009},
  volume={398},
  pages={263-270}
}
  • D. Majaess, D. Turner, D. Lane
  • Published 2009
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • ABSTRACT Classical and Type II Cepheids are used to reinvestigate specific properties of theGalaxy.A new TypeII reddening-freeCepheid distance parameterizationis formulatedfrom LMC Cepheids (OGLE), with uncertainties typically no larger than 5–15%. Adistance to the Galactic centre of R 0 = 7.8 ± 0.6 kpc is derived from the mediandistance to Type II Cepheids in the bulge (OGLE), R 0 = 7.7±0.7 kpc from a distanceto the near side of the bulge combined with an estimated bulge radius of 1.3 ± 0.3kpc… CONTINUE READING
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    References

    SHOWING 1-10 OF 111 REFERENCES
    The Discovery of Cepheids and a Distance to NGC 5128
    • 78
    • PDF
    Cepheid parallaxes and the Hubble constant
    • 162
    • Highly Influential
    • PDF
    Cepheids as Distance Indicators
    • 121
    The Cepheids of Population II and Related Stars
    • 97
    THE DISTANCE SCALE FOR CLASSICAL CEPHEID VARIABLES
    • 52
    The distance to the Galactic Centre based on Population-II Cepheids and RR Lyrae stars
    • 80
    • Highly Influential
    • PDF