Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...231l..11d&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 231, no. 2, May 1990, p. L11-L14. Research supported by the European Southern
Astronomy and Astrophysics
Astrophysics
7
Astronomical Photometry, Emission Spectra, Planetary Nebulae, Wolf-Rayet Stars, Forbidden Transitions, Oxygen Spectra, Stellar Magnitude, Stellar Mass Ejection, Ubv Spectra
Scientific paper
Direct imaging, photometry, and optical and mm-spectroscopy of We 21
shows that this object is a subluminous WN 8 star with an absolute
magnitude near Mv = -1.3. It is the central star of a low-excitation,
possibly nitrogen-rich planetary nebula, which interacts with dense
interstellar material of the inner Carina arm.
Duerbeck Hilman W.
Reipurth Bo
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