Molecule and Dust Formation in Novae

1994 
Observations of CO emission in Nova Sco 1992 are discussed. Observations of CO in this and other novae, notably NQ Vul (Nova Vul 1976) suggest that CO formation is a necessary precursor to the formation of an optically thick dust shell.
    • Correction
    • Source
    • Cite
    • Save
    • Machine Reading By IdeaReader
    8
    References
    0
    Citations
    NaN
    KQI
    []