The peculiar planetary nebula Abell 35

Details The peculiar planetary nebula Abell 35 The peculiar planetary nebula Abell 35

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...244..903j&link_type=abstract

Astrophysical Journal, Part 1, vol. 244, Mar. 15, 1981, p. 903-911.

Astronomy and Astrophysics

Astrophysics

66

Binary Stars, Emission Spectra, Planetary Nebulae, Stellar Spectrophotometry, Stellar Winds, Astronomical Photography, Forbidden Bands, H Alpha Line, Infrared Spectra, Interstellar Matter, Oxygen, Stellar Mass Ejection, Ubv Spectra

Scientific paper

The planetary nebula Abell 35 appears strikingly different when photographed in forbidden O III as compared to its H-alpha image. The disparity is believed to be due to the effects of a stellar wind originating with a binary central star interacting with the nebular shell. The previously unidentified central star is shown to have a transverse velocity of 150 km/s and exhibits a wind having a terminal velocity of 185 km/s at a mass-loss rate of 3 x 10 to the -9th solar masses per year. The distance to the nebula is 360 pc, as determined photometrically from the visible member of the binary nucleus.

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