Reddening maps of the LMC and SMC are produced via SED fitting of RGB stars from SMASH and VMC photometry, yielding mean E(B-V) of 0.076 mag and 0.058 mag with relative spatial structure stable across three stellar atmosphere models but absolute values differing by up to 0.03 mag.
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3 Pith papers cite this work. Polarity classification is still indexing.
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A joint convective coupling index shows moderate, age-dependent correlation with rotation periods of solar-mass stars, stronger in younger objects and weaker later.
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.
citing papers explorer
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Reddening maps of the Magellanic Clouds using spectral energy distribution fitting of red giants
Reddening maps of the LMC and SMC are produced via SED fitting of RGB stars from SMASH and VMC photometry, yielding mean E(B-V) of 0.076 mag and 0.058 mag with relative spatial structure stable across three stellar atmosphere models but absolute values differing by up to 0.03 mag.
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How plasma coupling and convective-zone depth shape the rotation of solar-mass stars
A joint convective coupling index shows moderate, age-dependent correlation with rotation periods of solar-mass stars, stronger in younger objects and weaker later.
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Characterizing six seismic solar analogs observed by Kepler, K2, and HERMES
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.