Detection of 17.26-day eclipses in KQ Puppis reveals it as a hierarchical triple with dynamical masses of ~10 M⊙ for the RSG and ~14 M⊙ for the inner pair, plus the first orbital parallax for any red supergiant.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
representative citing papers
Buoyancy glitches in the Brunt-Väisälä frequency and evanescent zone contribute to the g-mode phase in red-giant stars beyond the usual ε_g reflection term, prompting a modified formula and new quantification formalism.
PlatoSim is an end-to-end simulator for PLATO's high-precision space photometry that models photon collection through optics and detectors to digital output.
citing papers explorer
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Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates
Detection of 17.26-day eclipses in KQ Puppis reveals it as a hierarchical triple with dynamical masses of ~10 M⊙ for the RSG and ~14 M⊙ for the inner pair, plus the first orbital parallax for any red supergiant.
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Facing the phase: Gravity-mode offset and buoyancy glitches in red--giant branch stars
Buoyancy glitches in the Brunt-Väisälä frequency and evanescent zone contribute to the g-mode phase in red-giant stars beyond the usual ε_g reflection term, prompting a modified formula and new quantification formalism.
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PlatoSim: An end-to-end PLATO camera simulator for modelling high-precision space-based photometry
PlatoSim is an end-to-end simulator for PLATO's high-precision space photometry that models photon collection through optics and detectors to digital output.