Three micron spectra of carbon stars in the Large Magellanic Cloud

Details Three micron spectra of carbon stars in the Large Magellanic Cloud Three micron spectra of carbon stars in the Large Magellanic Cloud

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..259m&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

Stars: Agb, Stars: Atmospheres, Galaxy: Magellanic Clouds

Scientific paper

Infrared spectra of six carbon-rich stars were obtained with the Very
Large Telescope (VLT). We found a metallicity dependence in the
equivalent width of the molecular bands, and we discuss the causes of
this.

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