Discovery and multi-wavelength follow-up of a new FU Orionis accretion outburst in V7995 Sgr with photometry and spectroscopy confirming the classification.
136o137 Samus', N.N., et al
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
representative citing papers
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.
C-rich AGB stars trace the Galactic warp with larger amplitudes than Cepheids at intermediate ages of about 1 Gyr.
Machine learning trained on Gaia DR2 parallaxes yields unbiased Tycho-2 to Johnson-Cousins magnitude transformations with accurate predicted uncertainties for 2.5 million stars.
citing papers explorer
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V7995 Sgr: A New FU Orionis Accretion Outburst Near NGC 6589/6590
Discovery and multi-wavelength follow-up of a new FU Orionis accretion outburst in V7995 Sgr with photometry and spectroscopy confirming the classification.
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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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Milky Way's warped disc traced by AGB stars
C-rich AGB stars trace the Galactic warp with larger amplitudes than Cepheids at intermediate ages of about 1 Gyr.
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Conversion of Tycho-2 to Johnson-Cousins Magnitudes in the Gaia Era
Machine learning trained on Gaia DR2 parallaxes yields unbiased Tycho-2 to Johnson-Cousins magnitude transformations with accurate predicted uncertainties for 2.5 million stars.