M (sub)Dwarf Model Atmospheres: The Next Generation
- 1 January 1995
- book chapter
- Published by Springer Nature
Abstract
No abstract availableKeywords
This publication has 16 references indexed in Scilit:
- The influence of H2O line blanketing on the spectra of cool dwarf starsThe Astrophysical Journal, 1994
- An infrared spectral sequence for M dwarfsMonthly Notices of the Royal Astronomical Society, 1994
- M dwarf spectra from 0.6 to 1.5 micron - A spectral sequence, model atmosphere fitting, and the temperature scaleThe Astrophysical Journal, 1993
- Infrared photometry and spectroscopy of the brown dwarf candidate PC0025+0447The Astronomical Journal, 1992
- Effective temperatures of M dwarfsThe Astrophysical Journal, 1992
- Band origins for water up to 22 000 cm−1: A comparison of spectroscopically determined potential energy surfacesJournal of Molecular Spectroscopy, 1991
- Theoretical models of very low mass stars and brown dwarfsThe Astrophysical Journal, 1989
- Transition rates for the TiO beta, delta, phi, gamma-prime, gamma, and alpha systemsThe Astrophysical Journal, 1986
- Evolution of very low mass stars and brown dwarfs. I - The minimum main-sequence mass and luminosityThe Astrophysical Journal, 1985
- The Infrared Opacity of Hot Water VaporThe Astrophysical Journal Supplement Series, 1967