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Evolved Massive Stars at Low Metallicity. VII. The Lower Mass Limit of the Red Supergiant Population in the Large Magellanic Cloud
Published 2024-01-01“…Here, we assemble a spectroscopic evolved cool star sample with 6602 targets, including RSGs, asymptotic giant branch stars, and red giant branch stars, in the Large Magellanic Cloud based on Gaia DR3 and Sloan Digital Sky Survey IV/APOGEE-2. …”
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Revised Architecture and Two New Super-Earths in the HD 134606 Planetary System
Published 2024-01-01“…HD 134606 now displays four low-mass planets in a compact region near the star, one gas giant further out in the habitable zone, an additional companion in the outer regime, and a low-mass M dwarf stellar companion at large separation, making it an intriguing target for system formation/evolution studies. …”
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Ba Enrichment in Gaia MS+WD Binaries: Tracing s-process Element Production
Published 2024-01-01Get full text
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Fitting Methods for Probability Distribution Functions in Turbulent Star-forming Clouds
Published 2025-01-01Get full text
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The Gemini NICI Planet-Finding Campaign: The Frequency of Giant Planets around Young B and A Stars
Published 2013“…Considering the contrast limits of our NICI data and the fact that we did not detect any planets, we use high-fidelity Monte Carlo simulations to show that fewer than 20% of 2 M_sun stars can have giant planets greater than 4 M_Jup between 59 and 460 AU at 95% confidence, and fewer than 10% of these stars can have a planet more massive than 10 M_Jup between 38 and 650 AU. …”
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Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226
Published 2016“…</p> <h4>Results</h4> <p>In addition to producing double white dwarf and double neutron star binaries, CE evolution may also produce massive BH-BH systems with individual BH component masses of up to ~50 60 M⊙, in particular for donor stars evolved to giants beyond the Hertzsprung gap. However, the physics of envelope ejection of massive stars remains uncertain. …”
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The Structure of the Molecular Envelope of the Ring Nebula (NGC 6720)
Published 2025-01-01“…We assert that the Ring’s molecular envelope represents the “fossil” remnant of a relatively sudden mass ejection ∼6000 yr ago that terminated the progenitor star’s asymptotic giant branch (AGB) evolution, and that this ellipsoidal envelope of AGB ejecta was then punctured by fast, collimated polar outflows or jets resulting from interactions between the progenitor and one or more companion stars. …”
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Searching for Barium Stars from the LAMOST Spectra Using the Machine-learning Method: I
Published 2023-01-01Get full text
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Age Analysis of Extrasolar Planets: Insight from Stellar Isochrone Models
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Calibrating the Color–Magnitude Relation of M Giants by Using Open Clusters
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TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf
Published 2023-01-01Get full text
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PHANGS–JWST First Results: Duration of the Early Phase of Massive Star Formation in NGC 628
Published 2023-01-01Get full text
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