Molecular Constituents Identified in the 3-4 μm Spectral Region of Cool Stars.

Details Molecular Constituents Identified in the 3-4 μm Spectral Region of Cool Stars. Molecular Constituents Identified in the 3-4 μm Spectral Region of Cool Stars.

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977baas....9..636r&link_type=gif

Bulletin of the American Astronomical Society, Vol. 9, p.636

Astronomy and Astrophysics

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