PHOST - Physics of Oscillating Stars (2018)
Binary systems anchor many of the fundamental relations relied upon in asteroseismology. Masses and radii are rarely constrained better than when measured via orbital dynamics and eclipse depths. Pulsating binaries have much to offer.
Murphy, Simon J.
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Precise orbital parameters,masses, and parallax of the subgiant binary system 12 Persei: a combined spectroscopic-interferometric analysis. [PDF]
Abushattal AA +8 more
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Scalable photonic-based nulling interferometry with the dispersed multi-baseline GLINT instrument. [PDF]
Martinod MA +15 more
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Red novae, their progenitors, and remnants. [PDF]
Kamiński T, Blagorodnova N.
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Light People: Professor James C. Wyant. [PDF]
Wang H, Yu C.
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The fragmentation properties of massive star-forming regions in 30Dor-10 at 2000 au resolution. [PDF]
Traficante A +11 more
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Discovery of a star sensitive to the spin of Sagittarius A. [PDF]
Abd El Dayem K +92 more
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Imaging black holes: a VLBI success story. [PDF]
Zensus JA.
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Rank-Based Detection of Gravitational-Wave Transients Using Chatterjee Correlation. [PDF]
Martinez DB +6 more
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SBAS-InSAR Based Deformation Monitoring of Tailings Dam: The Case Study of the Dexing Copper Mine No.4 Tailings Dam. [PDF]
Xie W, Wu J, Gao H, Chen J, He Y.
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