Laboratory Production of the λ 4050 Group Occurring in Cometary Spectra; Future Evidence for the Presence of CH2 Molecules in Comets.

Details Laboratory Production of the λ 4050 Group Occurring in Cometary Spectra; Future Evidence for the Presence of CH2 Molecules in Comets. Laboratory Production of the λ 4050 Group Occurring in Cometary Spectra; Future Evidence for the Presence of CH2 Molecules in Comets.

Sep 1942

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1942apj....96..314h&link_type=gif

Astrophysical Journal, vol. 96, p.314-315

Astronomy and Astrophysics

Astrophysics

23

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