Equivalent Width of Molecular Lines in Stars. III: Lines of Lyman Band of H2 and (A-X) Band of CO and SiO in Stars

Details Equivalent Width of Molecular Lines in Stars. III: Lines of Lyman Band of H2 and (A-X) Band of CO and SiO in Stars Equivalent Width of Molecular Lines in Stars. III: Lines of Lyman Band of H2 and (A-X) Band of CO and SiO in Stars

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..49..389k&link_type=abstract

Astrophysics and Space Science, Volume 49, Issue 2, pp.389-398

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have calculated the expected equivalent widths of the individual rotational lines of the Lyman band of H2 and (A-X) band of CO and SiO for Main Sequence stars. The results indicate that the lines of H2 should be observable in absorption up toT e≲9000 K. The lines of CO are found to be much weaker than those of H2 lines. A discussion of these results is presented.

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