The OB associations of 30 Doradus in the Large Magellanic Cloud. I - Stellar observations and data reductions

@article{Parker1993TheOA,
  title={The OB associations of 30 Doradus in the Large Magellanic Cloud. I - Stellar observations and data reductions},
  author={J. Parker},
  journal={The Astronomical Journal},
  year={1993},
  volume={106},
  pages={560-577}
}
  • J. Parker
  • Published 1993
  • Physics
  • The Astronomical Journal
UBV photometry is presented for 2400 stars in the OB associations of 30 Doradus in the Large Magellanic Cloud, and I discuss new spectroscopic observations of 54 stars including 24 O stars. The CCD fields cover an area of 50 square arcminutes in the central region. The entire catalog (exclusive of the dense core cluster R 136) is photometrically complete to V = B = 18 mag and U = 17 mag, although the completeness magnitudes are fainter for regions with less nebular contamination. 
A Double Cluster at the Core of 30 Doradus
Gemini/GMOS detection of stellar velocity variations in the ionising cluster of 30 Dor
VLT‐MAD observations of the core of 30 Doradus
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