Infrared Observations of Large Amplitude Pulsating Stars
| dc.creator | Whitelock, Patricia A. | |
| dc.date | 1997-10-02 | |
| dc.date.accessioned | 2026-07-07T02:24:24Z | |
| dc.date.available | 2026-07-07T02:24:24Z | |
| dc.description | Our understanding of large amplitude pulsating stars and their status in stellar evolution is briefly reviewed. The paper then describes the near-infrared light curves of various asymptotic giant branch stars, concentrating on possible evidence for changing mass-loss rates. The stars discussed include oxygen- and carbon-rich Miras, OH/IR stars, thick-shelled carbon stars and symbiotic Miras. Finally a newly discovered Mira variable in the Sagittarius Dwarf Galaxy is described. | |
| dc.description | Invited Review for JD24 at IAU General Assembly, to appear in: Pulsating Stars - Recent Developments in Theory and Observation, (eds.) M. Takeuti & D. Sasselov, Universal Academic Press, Tokyo. 12 Pages, 6 postscript figures, LaTeX, requires jd24.sty | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9710032 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9710032 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11605 | |
| dc.subject | Astrophysics | |
| dc.title | Infrared Observations of Large Amplitude Pulsating Stars | |
| dc.type | text |