He2-36 - A planetary nebula with a high velocity jet?

Details He2-36 - A planetary nebula with a high velocity jet? He2-36 - A planetary nebula with a high velocity jet?

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aj.....90.2550f&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 90, Dec. 1985, p. 2550-2554.

Astronomy and Astrophysics

Astronomy

8

A Stars, Astronomical Spectroscopy, Companion Stars, Planetary Nebulae, Ultraviolet Astronomy, Emission Spectra, Iue, Jets, Line Spectra

Scientific paper

The ultraviolet spectrum of the planetary nebula He2-36 was observed in the low-dispersion mode of the IUE. Strong emission lines of C III], He II, and C IV are observed, as well as some weak lines and a moderately strong stellar continuum, suggesting a hot companion to the visual A2 III central star. The extinction to He2-36 was determined from the He II I(λ1640)/I(λ4686) ratio. The C IV line has an unusual split structure. If the λ1545 component is due to a blueshifted component from the "jet" emanating from the nebula, its velocity would be -600 km s-1, which is unique for a planetary nebula.

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