Dust features of visually bright AGB variables as seen by ISO and IRAS
- Author(s)
- Josef Hron, Rita Loidl, Franz Kerschbaum
- Abstract
ISO-SWS spectra of two Mira variables (R Cas and T Dra), taken at two different pulsational phases, are presented. We describe the reduction of the data and the encountered problems. The dust features observed by ISO at different phases and with the Low Resolution Spectrometer of IRAS are compared. We briefly discuss the results in terms of current models for the circumstellar dust shells of AGB variables.
- Organisation(s)
- Department of Astrophysics
- Journal
- Astrophysics and Space Science
- Volume
- 251
- Pages
- 211-214
- No. of pages
- 4
- ISSN
- 0004-640X
- DOI
- https://doi.org/10.1007/978-94-017-1307-8_30
- Publication date
- 1997
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103003 Astronomy
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/dust-features-of-visually-bright-agb-variables-as-seen-by-iso-and-iras(47e8c710-1a69-4691-999e-4ea08a4ac428).html