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Neutral oxygen in planetary nebulae - Probing radiative transfer and nebular structure

Journal Article · · Astrophysical Journal; (United States)
DOI:https://doi.org/10.1086/170348· OSTI ID:5157220
; ;  [1]
  1. Toronto, University (Canada) York University, North York (Canada) Canadian Institute for Theoretical Astrophysics, Toronto (Canada)
For the first time, forbidden O I 5577 A and forbidden O I 6364 A have together been mapped across planetary nebulae, making possible direct measurement of transition zone temperatures. In NGC 2440, the neutral oxygen temperature is 10,400 {plus minus} 600 K, compared with 10,200 {plus minus} 200 K for the forbidden N II temperature and 14,100 {plus minus} 300 K for the forbidden O III temperature. The forbidden O I temperature in NGC 3918 is 13,000 {plus minus} 900 K, significantly different from that in NGC 2440. Models computed with the nebula code CLOUDY successfully reproduce the forbidden O I and forbidden O III temperatures observed in NGC 2440, indicating that the implemented blend of on-the-spot and outward-only approximations to the transfer of diffuse radiation is a reasonable representation of reality. Even though radiation hardening enhances the heating at large optical depths within a planetary nebula, an increase in the cooling efficiency can present a concomitant rise in temperature. It is predicted that hot transition zones, as observed in NGC 3918, should be restricted to nebulae with cooler central stars and metal abundances (particularly N) at or below solar. 48 refs.
OSTI ID:
5157220
Journal Information:
Astrophysical Journal; (United States), Journal Name: Astrophysical Journal; (United States) Vol. 377; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English