Detection of the Canis Major galaxy at (l;b) = (244°; −8°) and in the background of Galactic open clusters

@article{Bellazzini2004DetectionOT,
  title={Detection of the Canis Major galaxy at (l;b) = (244°; −8°) and in the background of Galactic open clusters},
  author={Michele Bellazzini and Rodrigo A. Ibata and Lorenzo Monaco and Nicolas Martin and Michael J. Irwin and Geraint F. Lewis},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2004},
  volume={354},
  pages={1263-1278}
}
We report on the detection of main-sequence stars belonging to the recently identified Canis Major (CMa) galaxy in a field located at ≃4.°2 from the centre of the stellar system. With main-sequence fitting we obtain a distance modulus (m - M) 0 = 14.5 ± 0.3 to the dwarf, corresponding to a distance of D ○. ≃ 8.0 ± 1.2 kpc, in full agreement with previous estimates based on the photometric parallax of M-giants. From the comparison with theoretical isochrones, we constrain the age of the main… Expand
Photometry of a Galactic Field at l = 232°, b = −6°: The Old Open Cluster Auner 1, the Norma-Cygnus Spiral Arm, and the Signature of the Warped Galactic Thick Disk
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