Discovery of the first carbon star in NGC 6822

Astronomy and Astrophysics – Astronomy

Scientific paper

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Carbon Stars, Local Group (Astronomy), Stellar Spectrophotometry, M Stars, Magellanic Clouds, Stellar Magnitude, Stellar Spectra

Scientific paper

A new photometric technique has been developed for detecting carbon and M stars in distant stellar systems, leading to isolation of carbon star candidates in a number of Local Group galaxies. One of the brighter candidates in NGC 6822 has been confirmed spectroscopically; at a distance of approximately 0.5 Mpc, it is the first truly extragalactic carbon star to be positively identified. The star has MI ≡ -5.7 mag, placing it near the upper luminosity end of known carbon stars in the Magellanic Clouds.

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