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- W4300852972 abstract "The study of molecules in planetary nebulae is still in its infancy; therefore, it is appropriate both to review existing knowledge and to anticipate developments that will arise as the subject matures. Briefly stated, this subject consists of observations of hydrogen, H 2 , and carbon monoxide, CO, molecules in a very few nebulae; the tentative identification of the hydrogen molecular ion, H 2 + ; unsuccessful searches for various other species; some theoretical work on molecular processes relevant to planetary nebulae; and the study of molecules in possible precursors of planetary nebulae. Such a facile summary might suggest that molecules are mere curiosities of peripheral interest; on the contrary, it can be asserted that molecular studies of planetary nebulae will yield important new information about their origins, structures, and evolution." @default.
- W4300852972 created "2022-10-04" @default.
- W4300852972 creator A5028480727 @default.
- W4300852972 date "1983-01-01" @default.
- W4300852972 modified "2023-09-23" @default.
- W4300852972 title "Molecules in Planetary Nebulae" @default.
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- W4300852972 doi "https://doi.org/10.1017/s0074180900093608" @default.
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