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Explore high-resolution observations of AGB stars using ALMA and SPHERE/VLT to understand dust formation, wind acceleration, and outflow mechanisms in oxygen-rich stellar environments.
Explore advanced polarimetric interferometry techniques and machine learning methods for reconstructing images of mass loss patterns in evolved stars using the VAMPIRES instrument.
Explore the R Cor Bor phenomenon through a new model explaining how dusty winds, molecular hydrogen clouds, and stellar evolution create mysterious stellar fading events.
Explore molecular emission patterns in high mass-loss rate AGB stars, focusing on salt molecules NaCl and KCl, and their implications for stellar wind chemistry and physics.
Explore groundbreaking research on Mira variables as distance indicators and their role in measuring the Hubble Constant, featuring new observations from HST and JWST in galaxy M101.
Delve into the analysis of S-type AGB stars' masses through pulsation period measurements, exploring third dredge-up thresholds and stellar evolution patterns in asymptotic giant branch stars.
Explore groundbreaking research on evolved stars within 3 kpc of the Sun, examining dust and gas return patterns through advanced instrumentation and data analysis techniques.
Explore the latest findings on polluted binary star systems, focusing on mass transfer from AGB stars to companions and the implications for stellar evolution and nucleosynthesis through observational data.
Explore stellar convection patterns and their role in astrophysical processes, from solar observations to recent findings about evolved stars and Red Supergiants using high-resolution imaging techniques.
Explore groundbreaking simulations of dust formation in binary star systems, focusing on common envelope interactions and their impact on stellar evolution and observational properties.
Explore modern red supergiant mass-loss rates and their effects on binary star systems, black hole formation, and gravitational wave sources detected by LIGO and Virgo.
Explore groundbreaking research on carbon-deficient red giants, revealing new insights about stellar mergers, luminosity patterns, and their connection to Li-rich giants through asteroseismology.
Explore how large-scale astronomical surveys revolutionize our understanding of evolved stars' mass loss, using statistical samples to improve stellar models and research methods.
Explore period-luminosity relationships of Galactic Miras through multi-epoch infrared observations, combining COBE/DIRBE and WISE data with AAVSO light curves to assess Gaia parallax precision.
Explore groundbreaking developments in particle accelerator technology, focusing on medical applications, compact designs, and innovative solutions for radiation therapy and proton beam delivery systems.
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