A period–luminosity–colour relation for Mira variables
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- Type
- article
- Published
- 1989-12-01
- Cited by
- 290
- References
- 0
- Access
- Open access
- OpenAlex
- https://openalex.org/W2118908971
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:122370788
Keywords
Physics, Astrophysics, Term (time), Luminosity, Globular cluster
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- Long-period Red Variables in the Large Magellanic Cloud from the MOA Database
- Pulsating Cool Stars and Galactic Structure
- Modelling the Spectral Energy Distributions of AGB Stars in the LMC
- The Distance and Orientation of the Galactic Bulge from Mira Variables: A. Preliminary Report
- 1.4. Miras as probes of the Galactic bulge
- Properties of AGB variables in the intermediate-age cluster NGC 419 in the SMC
- Physics and Chemistry of Circumstellar Dust Shells
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- Mid-infrared period–magnitude relations for AGB stars
- Three-component modeling of C-rich AGB star winds - II. The effects of drift in long-period variables
- Carbon Stars in the Sagittarius Dwarf Galaxy
- MACHO observations of LMC red giants: Mira and semi-regular pulsators, and contact and semi-detached binaries
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