35 AGB stars show iso-dom SiO maser spectra explained by third dredge-up plus low turbulence velocity enabling line-overlap pumping.
K., & Szyma´nski, G
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Simulations predict Roman will detect roughly 11,000 microlensing events including about 100 with isolated neutron star lenses, using a characteristic feature in log t_E versus log theta_E space for classification.
citing papers explorer
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29SiO and 30SiO J=1--0 maser signatures in Galactic AGB stars: the impact of third dredge up and turbulence velocity
35 AGB stars show iso-dom SiO maser spectra explained by third dredge-up plus low turbulence velocity enabling line-overlap pumping.
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Astrometric microlensing probes of the isolated neutron star population with Roman
Simulations predict Roman will detect roughly 11,000 microlensing events including about 100 with isolated neutron star lenses, using a characteristic feature in log t_E versus log theta_E space for classification.