Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...376..978k&link_type=abstract
Astronomy and Astrophysics, v.376, p.978-981 (2001)
Astronomy and Astrophysics
Astrophysics
2
Planetary Nebulae: General: Early Type Stars, Stars: Emission Lines, Be Stars: Individual: Th4-4, Stars: Evolution
Scientific paper
The first optical spectra of Th4-4, obtained by the author in 1970, showed strong continuum and broad HI emission lines. In other words, at this time the object looked like a Be star. Some years later, [OIII] emission lines appeared in the spectrum indicating the existence of a gaseous envelope. Today the optical spectrum of Th4-4 is quite similar to that of a moderate excitation planetary nebula. The magnitude of the object has dropped from V=14fm 4 to 16fm 6, and the effective temperature of the central star has increased from 22 000 K up to 40 000 K within the last 30 years.
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