Summary: A&A manuscript no.
(will be inserted by hand later)
Your thesaurus codes are:
06(08.16.4; 08.03.1; 08.09.2; R For; 08.13.2)
ASTRONOMY
AND
ASTROPHYSICS
November 17, 1998
Modelling the Spectral Energy Distribution and SED variability of
the Carbon Mira R Fornacis ?
A. Lobel 1 , J.G. Doyle 1 and S. Bagnulo 2
1 Armagh Observatory, College Hill Armagh BT61 9DG, N. Ireland
2 Institut f˜ur Astronomie, Universit˜at Wien T˜urkenschanzstrasse 17, A­1180 Wien, Austria
2 July 1998, Accepted date
Abstract. We have developed a new method to determine the
physical properties and the local circumstances of dust shells
surrounding Carbon­ and Oxygen­rich stars for a given pul­
sation phase. The observed mid­IR dust emission feature(s),
in conjunction with IRAS BB photometry and coeval optical
and near­IR BB photometry, are modelled from radiative trans­

Source: Armagh Observatory

Collections: Physics