Distances to Local Group Galaxies

@article{Walker2003DistancesTL,
  title={Distances to Local Group Galaxies},
  author={Alistair R. Walker},
  journal={arXiv: Astrophysics},
  year={2003},
  volume={635},
  pages={265-279}
}
  • A. Walker
  • Published 1 March 2003
  • Physics
  • arXiv: Astrophysics
Distances to galaxies in the Local Group are reviewed. In particular, the distance to the Large Magellanic Cloud is found to be (m − M) = 18.52 ± 0.10, corresponding to 50,600 ± 2,400 pc. The importance of M31 as an analog of the galaxies observed at greater distances is stressed, while the variety of star formation and chemical enrichment histories displayed by Local Group galaxies allows critical evaluation of the calibrations of the various distance indicators in a variety of environments. 

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References

SHOWING 1-10 OF 11 REFERENCES
Evolutionary Histories of Dwarf Galaxies in the Local Group
The star formation histories of Local Group (LG) dwarf galaxies and more distant potential LG members are reviewed. Problems in defining the spatial extent of the LG and membership are brieflyExpand
The Distances of the Magellanic Clouds
The present status of our knowledge of the distances to the Magellanic Clouds is evaluated from a post-Hipparcos perspective. After a brief summary of the effects of structure, reddening, age, andExpand
A Survey of M31 Globular Clusters using WFPC2 on board HST
We report new, as yet unpublished HST/WFPC2 V, I photometry of 9 globular clusters in M31. These are part of a total sample of 19 clusters on M31 with well observed CMDs from HST. The clusters haveExpand
Luminosities of AGB Variables
The prevailing evidence suggests that most large-amplitude AGB variables follow the period luminosity (PL) relation that has been established for Miras in the LMC and galactic globular clusters.Expand
The Distance to the Large Magellanic Cloud; A Critical Review
Five independent methods of deriving the distance modulus of the Large Magellanic Cloud are reviewed and compared. A value in the range 18.60 to 18.80 is presently preferred.
The Local Group, (Cambridge
  • 2000
Gieren: this volume
  • 2003
Distance Scales and the Local Group
3-D Visualization of the Intrinsic Shape of the SMC
...
1
2
...