The nature of a nebulous stellar object in Centaurus

Details The nature of a nebulous stellar object in Centaurus The nature of a nebulous stellar object in Centaurus

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rmxaa..15...85m&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica (ISSN 0185-1101), vol. 15, Dec. 1987, p. 85-88.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Centaurus Constellation, Giant Stars, Stellar Envelopes, Stellar Evolution, Color-Magnitude Diagram, Early Stars, Infrared Astronomy Satellite, Ubv Spectra

Scientific paper

A nebulous stellar object found by Vogt et al. (1981) has been studied
further in order to determine its real nature. The authors conclude that
this object is not a young pre-main sequence star, but that it is a star
evolving away from the main sequence probably towards the asymptotic
giant branch region.

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