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HST-NICMOS observations of extensive triggered star formation within the 30 Doradus Nebula

Published online by Cambridge University Press:  25 May 2016


Nolan R. Walborn
Affiliation:
Space Telescope Science Institute, Baltimore, MD 21218, USA
Rodolfo H. Barbá
Affiliation:
Space Telescope Science Institute, Baltimore, MD 21218, USA


Abstract

The extensive ‘second generation’ of star formation within the 30 Doradus Nebula, evidently triggered by the R136 central cluster around its periphery, has been imaged with HST-NICMOS. Many new infrared sources and structures are found in these images.


Type
Part 4. Wolf-Rayet stars and other hot massive stars in the Galactic Center and in Local Group giant H II regions (individual stars)
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Rubio, M., Barbá, R., Walborn, N.R., Probst, R.G., et al. 1998, AJ 116, 1708 CrossRefGoogle Scholar
Massey, P., Hunter, D.A. 1998, ApJ 493, 180 CrossRefGoogle Scholar
Scowen, P.A., Hester, J.J., Sankrit, R., Gallagher, J.S., et al. 1998, AJ 116, 163 CrossRefGoogle Scholar
Walborn, N.R, Barbá, R., Brandner, W., Rubio, M., et al. 1999, AJ 117, 255 CrossRefGoogle Scholar
Walborn, N.R., Blades, J.C. 1997, ApJS 112, 457 CrossRefGoogle Scholar
Walborn, N.R., Parker, J.Wm. 1992, ApJ 399, L87 CrossRefGoogle Scholar

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HST-NICMOS observations of extensive triggered star formation within the 30 Doradus Nebula
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