A new bipolar nebula in Centaurus

Details A new bipolar nebula in Centaurus A new bipolar nebula in Centaurus

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.188..327w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 188, Aug. 1979, p. 327-330.

Astronomy and Astrophysics

Astronomy

10

Astronomical Spectroscopy, Infrared Astronomy, Interstellar Gas, Nebulae, Cosmic Dust, Late Stars, Morphology, Photographic Plates, Stellar Envelopes

Scientific paper

A new bipolar or butterfly-shaped nebula has been discovered and shown
to have an infrared excess. The spectra of the central object and wings
are of similar type, around G0. No emission lines are apparent. The
infrared excess appears to be due to thermal emission from dust.

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