Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-10-21
ApJ, 532, 384
Astronomy and Astrophysics
Astrophysics
36 pages, 8 tables, 7 figures, accepted for publication in ApJ
Scientific paper
10.1086/308536
In this paper we study new infrared spectra of the evolved planetary nebula NGC 6445 obtained with ISO. These data show that the thermal emission from the grains is very cool and has a low flux compared to H beta. A model of the ionized region is constructed, using the photo-ionization code CLOUDY 90.05. Based on this model, we show from depletions in the gas phase elements that little grain destruction can have occurred in the ionized region of NGC 6445. We also argue that dust-gas separation in the nebula is not plausible. The most likely conclusion is that grains are residing inside the ionized region of NGC 6445 and that the low temperature and flux of the grain emission are caused by the low luminosity of the central star and the low optical depth of the grains. This implies that the bulk of the silicon-bearing grains in this nebula were able to survive exposure to hard UV photons for at least several thousands of years, contradicting previously published results. A comparison between optical and infrared diagnostic line ratios gives a marginal indication for the presence of a t^2-effect in the nebula. However, the evidence is not convincing and other explanations for the discrepancy are also plausible. The off-source spectrum taken with ISO-LWS clearly shows the presence of a warm cirrus component with a temperature of 24 K as well as a very cold component with a temperature of 7 K. Since our observation encompasses only a small region of the sky, it is not clear how extended the 7 K component is and whether it contributed significantly to the FIRAS spectrum taken by COBE. Because our line of sight is in the galactic plane, the very cold component could be a starless core.
G.
J.
Beintema Douwe A.
de Steene Griet C. Van
Ferland
No associations
LandOfFree
Properties of Dust Grains in Planetary Nebulae - I. The Ionized Region of NGC 6445 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 Properties of Dust Grains in Planetary Nebulae - I. The Ionized Region of NGC 6445, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Properties of Dust Grains in Planetary Nebulae - I. The Ionized Region of NGC 6445 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-426604