OH/IR stars: Very long period variables with extreme mass loss rates on their nature and their distribution in the galaxy
- 31 July 1985
- journal article
- review article
- Published by Elsevier in Physics Reports
- Vol. 124 (4) , 255-314
- https://doi.org/10.1016/0370-1573(85)90095-x
Abstract
No abstract availableKeywords
This publication has 79 references indexed in Scilit:
- Luminosities and mass loss rates of OH/H2O maser starsThe Astrophysical Journal, 1984
- Extended OH maser emission from circumstellar shells and the envelope around OH 26.5 + 0.6The Astrophysical Journal, 1981
- The universe at faint magnitudes. I - Models for the galaxy and the predicted star countsThe Astrophysical Journal Supplement Series, 1980
- UBVRI photometry. II - The Cousins VRI system, its temperature and absolute flux calibration, and relevance for two-dimensional photometryPublications of the Astronomical Society of the Pacific, 1979
- Multibaseline VLBI observations of the 1612 MHz OH masers toward NML Cygni and VY Canis MajorisThe Astrophysical Journal, 1979
- The asymptotic giant branch evolution of intermediate-mass stars as a function of mass and composition. I - Through the second dredge-up phaseThe Astrophysical Journal, 1979
- Infrared observations of the galactic center. IV - The interstellar extinctionThe Astrophysical Journal, 1978
- Is there a maser in the silicon monoxide ground stateThe Astrophysical Journal, 1975
- Energy spectra of the stars.The Astrophysical Journal, 1929
- Radiometer measurements of stellar energy spectra.The Astrophysical Journal, 1924