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How to disentangle geometry and mass-loss rate from AGB-star spectral energy distributions. The case of EP Aquarii
How to disentangle geometry and mass-loss rate from AGB-star spectral energy distributions. The case of EP Aquarii
2020
J. Wiegert
M. A. T. Groenewegen
Alain Jorissen
L. Decin
T. Danilovich
Keywords:
Spectral density
Physics
Asymptotic giant branch
Astrophysics
loss rate
Correction
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