The variable mass-loss in low-mass red giant stars: Chromospheric motion across stellar evolution in 47 Tuc
astro-ph.SR, astro-ph.GA
Submitted: 2026-10-03
Updated: 2026-10-03
Code: https://github.com/Inebama/FLAMES-MOS-pipeline-reduction
Sources
- The Chemical Composition of the Sun
- A New Catalog of Globular Clusters in the Milky Way
- A compilation of solar atlases (from Delbouille, Kurucz, Gandorfer, Stenflo) at disk centre and at limb from $\lambda$ 3000 {\AA} to $\lambda$ 8800 {\AA}
- The Stellar Winds Atlas I: Current uncertainties in mass-loss rates
- Compendium solar spectrum formation
- Fifty Years of CAK
Related papers
- HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
- Effect of Neutron Star Jets on Common Envelope Evolution
- Constraining the origin of magnetic white dwarfs
- JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
- Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
- Can MHD Oscillations Modulate Quasi-Periodic Plasma Release from Coronal Streamers?