W 16-185 - A heavily reddened, low-excitation planetary nebula

Details W 16-185 - A heavily reddened, low-excitation planetary nebula W 16-185 - A heavily reddened, low-excitation planetary nebula

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..867n&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 690, p. 867-870.

Astronomy and Astrophysics

Astronomy

1

Interstellar Extinction, Planetary Nebulae, Stellar Spectrophotometry, Charge Coupled Devices, Emission Spectra, H Ii Regions, Line Spectra, Point Sources, Stellar Color

Scientific paper

Low-dispersion spectroscopy and narrow-band CCD imaging has been obtained for the planetary nebula (PN) candidate W 16-185 in order to clarify its nature. These data, in particular the emission-line spectrum, lead to the conclusion that it is a heavily reddened, low-excitation PN rather than a compact H II region. However, the IRAS luminosity and colors of the associated point source are rather unusual for a PN.

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