New light on dark stars : red dwarfs, low-mass stars, brown dwarfs

By I. Neill Reid, S. Hawley. 2000

203 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/4acb0d863d23fd51e65c045ac21b7458a0327231

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THE CALIFORNIA PLANET SURVEY. I. FOUR NEW GIANT EXOPLANETS (2010, background): “Second, we find that the M dwarf Gl 661B has nearly identical NIR absolute magnitudes to HD126614B (Table 6; Reid & Hawley 2005).”
THE BROWN DWARF KINEMATICS PROJECT I. PROPER MOTIONS AND TANGENTIAL VELOCITIES FOR A LARGE SAMPLE OF LATE-TYPE M, L, AND T DWARFS (2008, background): “The more informative number in this case is the median Vtan which, at 56 km/s, is nearly twice the expected value for the thin disk (see Reid & Hawley 2005).”
Characterization of M, L, and T Dwarfs in the Sloan Digital Sky Survey (2002, methodology): “Numerous instances of incorrect fitting that propagated into incorrect luminosity and mass function determinations, exist in the literature (see Reid & Hawley 2000).”
Low-Mass Dwarf Template Spectra from the Sloan Digital Sky Survey (2006, background): “…interesting constraints on the structure of the atmosphere, suggesting that the formation of TiO, thought to take place near the temperature minimum region below the chromospheric temperature rise (Chabrier et al. 2005; Reid & Hawley 2005), is affected by the presence of an overlying chromosphere.”
Testing LMC Microlensing Scenarios: The Discrimination Power of the SuperMACHO Microlensing Survey (2005, methodology): “We calculate Nobs and Et independently for each field and amplifier, as described below.”
Identification of New M Dwarfs in the Solar Neighborhood (2003, background): “The turbulent dynamo (Durney et al. 1993), however, appears to explain the stellar physics in such stars well, since it does not require a radiative-convective boundary layer and can produce magnetic fields by random convection motions in the convection zone (Reid & Hawley 2000).”
Discovery and Characterization of Transiting Super Earths Using an All-Sky Transit Survey and Follow-up by the James Webb Space Telescope (2009, methodology): “We convert spectral type to T eff , stellar mass and radius, using Table 4.1 of Reid & Hawley (2000).”
TRANSITS OF EARTH-LIKE PLANETS (2009, methodology): “In column 6, the absolute visual magnitude M is derived from the V-I value and a plot of measured values of M vs (V-I) (Reid & Hawley 2005, Reid et al. 1995).”
Stellar Multiplicity (2013, background): “3.2.5 High-order multiple systems The ratio of multiple to binary systems among low-mass stars is ≈ 21% (Reid & Hawley 2005), similar to the ratio observed for solartype stars.”