PN G160.7-2.9: A new planetary nebula

Details PN G160.7-2.9: A new planetary nebula PN G160.7-2.9: A new planetary nebula

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...282..197w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 282, no. 1, p. 197-198

Astronomy and Astrophysics

Astronomy

2

Astronomical Spectroscopy, Emission Spectra, H Alpha Line, Planetary Nebulae, Sky Surveys (Astronomy), Astronomical Photography, Stellar Evolution, Visible Spectrum

Scientific paper

A new planetary nebula (PNe) has been discovered during an extensive search for optically detectable galaxies in the zone of avoidance. The nebula (angular diameter = 25 sec) has a very low surface brightness and a strikingly smooth appearance, is highly evolved and lacks a visible central star up to mb = 21. A spectrum shows emission lines of H-alpha + (NII), (OIII), and possibly (SII).

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