Near-infrared spectral evolution of blue LMC clusters: a comparison with Galactic open clusters.

Details Near-infrared spectral evolution of blue LMC clusters: a comparison with Galactic open clusters. Near-infrared spectral evolution of blue LMC clusters: a comparison with Galactic open clusters.

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990rmxaa..21..202b&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 21, p. 202 - 206

Astronomy and Astrophysics

Astronomy

2

Open Clusters: Magellanic Clouds, Open Clusters: Spectra, Open Clusters: Ages

Scientific paper

The authors compare the spectral properties of young LMC clusters classified in age groups with the composite HR diagrams of Galactic open clusters from Mermilliod (1981). There is a strong correspondence between these evolutionary sequences in terms of phases in the stellar evolution, such as red supergiants, giants with origin in intermediate mass progenitors and Be stars.

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