Add to ORKGI will be reviewing three methods to identify late-type giants in extragalactic systems, based on the main characteristics of AGB stars (they are infrared bright, variable, and have spectral peculiarities)
Asymptotic Giant Branch (AGB) stars are important players in the chemical evolution modelling of gal...
Man’s interest in stars and stardust roots not only to better understand the Universewe live in but ...
Asymptotic giant branch (AGB) stars are simultaneously one of the most important and least well unde...
Context. The asymptotic giant branch (AGB) phase is characterised by substantial mass loss that is a...
Context. The asymptotic giant branch (AGB) phase is characterised by substantial mass loss that is a...
Asymptotic giant branch stars are essential contributors to the near and mid-IR emission of intermed...
Post-AGB stars evolve on a very fast track and hence not many are known. Their spectral properties m...
Context. Asymptotic giant branch (AGB) phases mark the end of the evolution for low- and intermediat...
Context. Asymptotic giant branch (AGB) phases mark the end of the evolution for low- and intermediat...
Context. Asymptotic giant branch (AGB) phases mark the end of the evolution for low- and intermediat...
Context. The asymptotic giant branch (AGB) phase is characterised by substantial mass loss that is ...
A review is presented of the most relevant results obtained in the last few years on this rare class...
We present a photometric analysis of the properties of asymptotic giant branch stars identified in t...
“The original publication is available at www.edpsciences.org/eas”. Copyright EAS/EDP Sciences.AGB s...
“The original publication is available at www.edpsciences.org/eas”. Copyright EAS/EDP Sciences.AGB s...
Asymptotic Giant Branch (AGB) stars are important players in the chemical evolution modelling of gal...
Man’s interest in stars and stardust roots not only to better understand the Universewe live in but ...
Asymptotic giant branch (AGB) stars are simultaneously one of the most important and least well unde...
Context. The asymptotic giant branch (AGB) phase is characterised by substantial mass loss that is a...
Context. The asymptotic giant branch (AGB) phase is characterised by substantial mass loss that is a...
Asymptotic giant branch stars are essential contributors to the near and mid-IR emission of intermed...
Post-AGB stars evolve on a very fast track and hence not many are known. Their spectral properties m...
Context. Asymptotic giant branch (AGB) phases mark the end of the evolution for low- and intermediat...
Context. Asymptotic giant branch (AGB) phases mark the end of the evolution for low- and intermediat...
Context. Asymptotic giant branch (AGB) phases mark the end of the evolution for low- and intermediat...
Context. The asymptotic giant branch (AGB) phase is characterised by substantial mass loss that is ...
A review is presented of the most relevant results obtained in the last few years on this rare class...
We present a photometric analysis of the properties of asymptotic giant branch stars identified in t...
“The original publication is available at www.edpsciences.org/eas”. Copyright EAS/EDP Sciences.AGB s...
“The original publication is available at www.edpsciences.org/eas”. Copyright EAS/EDP Sciences.AGB s...
Asymptotic Giant Branch (AGB) stars are important players in the chemical evolution modelling of gal...
Man’s interest in stars and stardust roots not only to better understand the Universewe live in but ...
Asymptotic giant branch (AGB) stars are simultaneously one of the most important and least well unde...