Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....94l..13p&link_type=abstract
Astronomy and Astrophysics, vol. 94, no. 2, Feb. 1981, p. L13-L16.
Astronomy and Astrophysics
Astrophysics
41
Astrometry, Hot Stars, Planetary Nebulae, Hertzsprung-Russell Diagram, Radii, Stellar Luminosity, Stellar Temperature
Scientific paper
A substantial fraction of the central stars are hot objects. The temperature of some of the hottest of the stars is investigated and found to be between 1O5°K and 6 × 105 °K. The radii and luminosities of these stars are found, and their evolution is discussed. In particular, some of the hottest of these stars are associated with recently formed nebulae, while others are substantially older.
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