Stellar Ionization of the Thermal Emission Regions in the Galactic Center

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Stanford University, 1995 - 330 pages

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Contents

A Preliminary Study
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1
27
19
36
Copyright

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Common terms and phrases

2.40 Wavelength absorption addition Arched Filaments average H-K band spectra Brackett lines broad band images Bry emission image Bry image Bry line central parsec cluster stars compact regions compact source data cube detected distribution of stars emission line stars Galactic Center galactic plane galaxy GG Car Güsten H band image H II regions H-K distribution hot stars hot young stars hydrogen indicate infrared interstellar extinction ionization Langer luminosity Maeder massive stars molecular cloud Najarro number distribution number of stars OB stars observations optically classified stars orbits photometry Pistol Source pixel presented in Figure radio emission regions regions H1-H8 RIGHT ASCENSION seen Sgr A East Sickle Position spectra of optically spectral type star formation Star Line Fluxes star WR stars located stellar winds Straight Filaments strong suggest supergiants Table Teff velocity Wavelength WN 6 stars Wolf-Rayet stars Yusef-Zadeh & Morris µm line

Bibliographic information

TitleStellar Ionization of the Thermal Emission Regions in the Galactic Center
AuthorAngela S. Cotera
ContributorStanford University. Department of Applied Physics
PublisherStanford University, 1995
Length330 pages
  
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