Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..445..325e&link_type=abstract
Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants. Proceedings of a conference held at University Ca
Astronomy and Astrophysics
Astronomy
Scientific paper
Dust is formed in the outer atmospheres and winds of AGB stars and severely affects their observed spectra and colours. Synthetic JHK colours from a grid of time-dependent C-star models are presented and compared to observed colours. The combined effects of pulsation and dust are significant, especially for the coolest and most luminous models. We are now extending the calculations with respect to effective temperature, luminosity, stellar mass, and pulsation amplitude, as well as the carbon excess.
Aringer Bernard
Eriksson Kimmo
Hofner Susanne
Nowotny Walter
Wachter Antonia
No associations
LandOfFree
Synthetic Colors for Dynamic C-Star Models 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 Synthetic Colors for Dynamic C-Star Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Synthetic Colors for Dynamic C-Star Models will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-829055