Equivalent width of molecular lines in stars

Details Equivalent width of molecular lines in stars Equivalent width of molecular lines in stars

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...41..301k&link_type=abstract

Solar Physics, Volume 41, Issue 2, pp.301-312

Physics

8

Scientific paper

The expected equivalent widths of the individual rotational lines of the
Lyman and Werner bands of the hydrogen molecule from the solar
atmosphere have been calculated. These results are used to predict what
one expects to observe with a specified wavelength bandpass. These are
compared with the observation of Dupree and Reeves.

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