Cool Stars, Stellar Systems and the Sun.

By E. Stempels. 2009

169 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/270ea92d3c24faf7c488e93ef6506c19abeb930a

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Citations in the corpus

• FORMATION AND EVOLUTION OF PLANETARY SYSTEMS: PROPERTIES OF DEBRIS DUST AROUND SOLAR-TYPE STARS (2008, background): “Analysis of IRAS data indicates that ∼ 15% of nearby AFGK type stars are surrounded by a debris disk with a dust-to-photosphere luminosity ratio exceeding that of the Vega debris disk (Backman & Gillett 1987; Plets & Vynckier 1999).”
• Confirmation of the Electron Cyclotron Maser Instability as the Dominant Source of Radio Emission from Very Low Mass Stars and Brown Dwarfs (2008, unknown): “40 10 v1 [ as tr oph ] 2 6 M ay 2 00 8 — stars: activity — stars: low-mass, brown dwarfs — stars: magnetic fields”
• A multiwavelength study of the M dwarf binary YY Geminorum (2015, methodology): “Multi-wavelength observations of flare activity on YY Gem were initiated by Jackson, Kundu & White (1989) using radio data from the VLA (see also, Gary, 1986).”
• Departures from LTE for neutral Li in late-type stars (2009, methodology): “Stellar lithium abundances are continuing to attract strong interest among the astronomical community.”
• Stellar magnetism: empirical trends with age and rotation (2014, background): “…regions f and the mean unsigned field strength in the regions BI (〈|BI |〉 = fBI), it is still debatable whether the saturation occurs in the filling factor f of magnetically active regions or in the stellar magnetism itself or in both (Solanki 1994; Saar 1996, 2001; Reiners, Basri & Browning 2009).”
• First stars VII - Lithium in extremely metal poor dwarfs (2006, background): “Interpretations by diffusion (Michaud 1986; Proffitt et al. 1990), rotationally induced mixing (Böhm-Vitense 2004; Talon & Charbonnel 2003; Pinsonneault et al. 1992), or mass loss (Schramm et al. 1990) have been proposed.”
• Asteroseismology of old open clusters with Kepler: direct estimate of the integrated red giant branch mass-loss in NGC 6791 and 6819 (2011, methodology): “(2007), who derived a very low average mass (M∼0.43±0.06 M⊙) for the luminous white dwarfs for which they obtained Keck/LRIS spectra, well below the limit for helium ignition in a degenerate core. In addition, the post-helium flash, helium-core-burning stars in this cluster are divided into a red gi”
• Non‐LTE line formation of Fe in late‐type stars – I. Standard stars with 1D and 〈3D〉 model atmospheres (2012, methodology): “The NLTE level populations of Fei and Feii were computed with an updated version of thedetail code (Butler & Giddings 1985) and multi (Carlsson 1986, 1992).”