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Citation-based clustering of publications using CitNetExplorer and VOSviewer. [PDF]
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A comprehensive search for hot subdwarf stars using Gaia and TESS I. Pulsating hot subdwarf B stars
Hot subdwarf B (sdB) stars are evolved, subluminous, helium-burning stars, most likely formed when red-giant stars lose their hydrogen envelope via interactions with close companions. They play an important role in our understanding of binary evolution, stellar atmospheres, and interiors.
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2MASS J035523.37+113343.7: A YOUNG, DUSTY, NEARBY, ISOLATED BROWN DWARF RESEMBLING A GIANT EXOPLANET. [PDF]
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Exploring central star variability of planetary nebulae using gaia photometry. [PDF]
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The Evolution of Compact Binary Star Systems. [PDF]
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