Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...283..165t&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 283, Aug. 1, 1984, p. 165-168.
Astronomy and Astrophysics
Astronomy
133
Balmer Series, Gas Ionization, Hydrogen Clouds, Main Sequence Stars, Stellar Spectra, Infrared Astronomy, Line Spectra, Lyman Spectra, Stellar Luminosity, Stellar Mass
Scientific paper
New calculations of the ionization from zero-age main-sequence (ZAMS) stars are presented. Ionization-bounded calculations for photoionization, both from the n = 1 and the n = 2 level of hydrogen, are presented. The n = 2 calculations are used to show that the suggestion of Balmer continuum ionization proposed by Simon et al. can account for the observed hydrogen-line excess in obscured ZAMS objects. The present results show that Balmer continuum ionization is more than adequate for the production of the observed excess.
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