Evolution of PAH Features from Proto- to Planetary Nebulae

Details Evolution of PAH Features from Proto- to Planetary Nebulae Evolution of PAH Features from Proto- to Planetary Nebulae

2005-10-11

arxiv.org/abs/astro-ph/0510306v1

AIP Conf.Proc.804:214-217,2006

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures, 1 table, to appear in the Proceedings of the conference "Planetary Nebulae as Astronomical Tools", edited

Scientific paper

10.1063/1.2146279

With the aim to investigate the overall evolution of UIR band features with hardening of UV radiation (increase of the star's effective temperature) we have analysed ISO spectra for 32 C-rich stars: 20 proto-planetary nebulae and 12 planetary nebulae with Wolf-Rayet central stars. In this contribution we discuss variations in the peak position of UIR bands among analysed objects, and demonstrate that variations in the ``7.7'' to 11.3 microns flux ratio are correlated with the effective temperature (probably due to an increase of the ionization state of their carriers).

Affiliated with

Also associated with

No associations

Rating

Evolution of PAH Features from Proto- to 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 Evolution of PAH Features from Proto- to Planetary Nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of PAH Features from Proto- to Planetary Nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-48336