Publication Date:
2019-06-28
Description:
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 M(I) = about -5.7 mag, placing it near the upper-luminosity end of known carbon stars in the Magellanic Clouds.
Keywords:
ASTRONOMY
Type:
Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X); 277; L9-L11
Format:
text