Infrared Observations of the Candidate LBV 1806-20 and Nearby Cluster Stars* ** ***
@article{Eikenberry2004InfraredOO, title={Infrared Observations of the Candidate LBV 1806-20 and Nearby Cluster Stars* ** ***}, author={S. Eikenberry and K. Matthews and J. LaVine and M. A. Garske and D. Hu and M. Jackson and S. Patel and D. Barry and M. Colonno and J. Houck and J. C. Wilson and S. Corbel and J. D. Smith}, journal={The Astrophysical Journal}, year={2004}, volume={616}, pages={506-518} }
We report near-infrared photometry, spectroscopy, and speckle imaging of the hot, luminous star we identify as candidate LBV 1806-20. We also present photometry and spectroscopy of three nearby stars, which are members of the same star cluster containing LBV 1806-20 and SGR 1806-20. The spectroscopy and photometry show that LBV 1806-20 is similar in many respects to the luminous Pistol star, albeit with some important differences. They also provide estimates of the effective temperature and… CONTINUE READING
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References
SHOWING 1-10 OF 40 REFERENCES
The connection between W31, SGR 1806-20, and LBV 1806-20: Distance, extinction, and structure
- Physics
- 2004
- 89
- PDF
Star Formation in R136: A Cluster of O3 Stars Revealed by Hubble Space Telescope Spectroscopy*
- Physics
- 1998
- 347
The Stellar Content of Obscured Galactic Giant H II Regions. III. W31
- Physics
- 2001
- 47
- Highly Influential
- PDF
Really Cool Stars and the Star Formation History at the Galactic Center
- Physics
- 2003
- 91
- Highly Influential
- PDF
The Discovery of an Embedded Cluster of High-Mass Stars near SGR 1900+14.
- Physics, Medicine
- The Astrophysical journal
- 2000
- 82
- PDF
JHKL Photometry and the K-Band Luminosity Function at the Galactic Center
- Physics
- 1996
- 107
- Highly Influential
- PDF