Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientific paper
2012-01-18
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
MNRAS accepted; 10 Figs
Scientific paper
We develop an approximate analytical solution for the transfer of line-averaged radiation in the hydrogen recombination lines for the ionized cavity and molecular shell of a spherically symmetric planetary nebula. The scattering problem is treated as a perturbation, using a mean intensity derived from a scattering-free solution. The analytical function was fitted to Halpha and Hbeta data from the planetary nebula NGC6537. The position of the maximum in the intensity profile produced consistent values for the radius of the cavity as a fraction of the radius of the dusty nebula: 0.21 for Halpha and 0.20 for Hbeta. Recovered optical depths were broadly consistent with observed optical extinction in the nebula, but the range of fit parameters in this case is evidence for a clumpy distribution of dust.
Gray Malcolm D.
Matsuura Mikako
Zijlstra Albert A.
No associations
LandOfFree
Radiation Transfer in the Cavity and Shell of Planetary Nebulae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Radiation Transfer in the Cavity and Shell of Planetary Nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiation Transfer in the Cavity and Shell of Planetary Nebulae will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-253399