ALMA Band 6 data detect SiO emission and masers up to v=8 in AGB stars, showing clumpy distributions, velocity gradients, and a tentative link between emission radius and mass-loss rate.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Gaia astrometry remains consistent with a binary origin for long secondary periods once sample contamination by semi-regular variables is accounted for.
citing papers explorer
-
ATOMIUM: Inner circumstellar envelopes of oxygen-rich AGB stars as revealed by highly excited SiO lines
ALMA Band 6 data detect SiO emission and masers up to v=8 in AGB stars, showing clumpy distributions, velocity gradients, and a tentative link between emission radius and mass-loss rate.
-
Eppur binaria non \'e esclusa: Gaia astrometry does not disfavor a binary origin for Long Secondary Periods
Gaia astrometry remains consistent with a binary origin for long secondary periods once sample contamination by semi-regular variables is accounted for.