The strengths of spectrum lines formed in stellar atmospheres with predominantly H- continuous absorption

Details The strengths of spectrum lines formed in stellar atmospheres with predominantly H- continuous absorption The strengths of spectrum lines formed in stellar atmospheres with predominantly H- continuous absorption

Jun 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964jqsrt...4..415w&link_type=ejournal

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 4, issue 3, pp. 415-426

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