NIR monitoring of star clusters in the Magellanic Clouds

Details NIR monitoring of star clusters in the Magellanic Clouds NIR monitoring of star clusters in the Magellanic Clouds

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..201t&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Agb, Variables, Stellar Evolution, Magellanic Clouds

Scientific paper

From the near-infrared monitoring observations of intermediate-age
clusters, we found that most AGB stars near the tip luminosity are
variables in the infrared. It is also suggested that their amplitude may
increase with their luminosities.

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