Spectral decomposition of 26 T Tauri disks finds Mg-rich silicate dust with 5-24% crystallinity and correlations linking annealed silica to stronger CO2 emission and forsterite to stronger H2O emission.
Mass accretion and planetary formation in young multiple stellar systems
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The paper reviews departures from classical binary evolution theory for low- and intermediate-mass stars, focusing on eccentric orbits, mass exchange, tides, and eccentricity maintenance.
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MINDS survey of silicates in T Tauri disks: Correlation between dust and gas
Spectral decomposition of 26 T Tauri disks finds Mg-rich silicate dust with 5-24% crystallinity and correlations linking annealed silica to stronger CO2 emission and forsterite to stronger H2O emission.
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Evolving Low- and Intermediate-Mass Binaries: Departures from Classical Theory
The paper reviews departures from classical binary evolution theory for low- and intermediate-mass stars, focusing on eccentric orbits, mass exchange, tides, and eccentricity maintenance.