H II REGION METALLICITY DISTRIBUTION IN THE MILKY WAY DISK
@article{Balser2011HIR, title={H II REGION METALLICITY DISTRIBUTION IN THE MILKY WAY DISK}, author={D. Balser and R. Rood and T. Bania and L. Anderson}, journal={The Astrophysical Journal}, year={2011}, volume={738}, pages={27} }
The distribution of metals in the Galaxy provides important information about galaxy formation and evolution. H II regions are the most luminous objects in the Milky Way at mid-infrared to radio wavelengths and can be seen across the entire Galactic disk. We used the National Radio Astronomy Observatory (NRAO) Green Bank Telescope to measure radio recombination line and continuum emission in 81 Galactic H II regions. We calculated LTE electron temperatures using these data. In thermal… Expand
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References
SHOWING 1-10 OF 127 REFERENCES
Carbon and Oxygen Galactic Gradients: Observational Values from H II Region Recombination Lines*
- Physics
- 2005
- 115
- Highly Influential
- PDF
THE ABUNDANCE SCATTER IN M33 FROM H II REGIONS: IS THERE ANY EVIDENCE FOR AZIMUTHAL METALLICITY VARIATIONS?*
- Physics
- 2011
- 61
- Highly Influential
- PDF
Galactic abundance gradients from Cepheids : On the iron abundance gradient around 10-12 kpc
- Physics
- 2008
- 65
- PDF