Dwarfs Cooler than “M”: The Definition of Spectral Type “L” Using Discoveries from the 2 Micron All‐Sky Survey (2MASS)
- 10 July 1999
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 519 (2), 802-833
- https://doi.org/10.1086/307414
Abstract
No abstract availableThis publication has 38 references indexed in Scilit:
- Chemical Equilibrium Abundances in Brown Dwarf and Extrasolar Giant Planet AtmospheresThe Astrophysical Journal, 1999
- The science of brown dwarfsReviews of Modern Physics, 1993
- The late-M dwarfsThe Astronomical Journal, 1991
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989
- A low-temperature companion to a white dwarf starNature, 1988
- JHKLM photometry - Standard systems, passbands, and intrinsic colorsPublications of the Astronomical Society of the Pacific, 1988
- Observations of M dwarfs beyond 2.2 mMonthly Notices of the Royal Astronomical Society, 1987
- New limits on the surface density of M dwarfs. I - Photographic survey and preliminary CCD dataThe Astronomical Journal, 1985
- 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
- Additional Note on ExcavationsThe Biblical Archaeologist, 1954