The problem of the n(e) and T-e fluctuations in the planetary nebulae (PN) in a view of the ISO data was investigated. The fluxes in the OIII fine structure (FS) lines for a large sample of PNe were estimated.

Original languageEnglish
Pages (from-to)513-514
Number of pages2
JournalAstrophysics and Space Science
Volume255
Issue number1-2
StatePublished - 1998
EventInternational Conference on ISOs View on Stellar Evolution - NOORDWIJKERHOUT, Netherlands
Duration: 1 Jul 19974 Jul 1997

    Research areas

  • planetary nebulae : temperature and density fluctuations, element abundances : CNO abundances, IR lines

ID: 49302170