Publication | Closed Access
The present status of four luminous variables in M 33
17
Citations
23
References
2006
Year
Cosmic AbundanceGalaxy FormationPhotometryM 33EngineeringHigh-energy AstrophysicsPhysicsCosmologyStellar StructurePhotometry (Optics)Massive StarsDark MatterChemical EvolutionLate Evolutionary Stages
Context. Understanding the origin of the instabilities of LBVs is important for shedding light on the late evolutionary stages of massive stars and on the chemical evolution of galaxies.
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