Kinematics and spectra of planetary nebulae with O VI-sequence nuclei

Details Kinematics and spectra of planetary nebulae with O VI-sequence nuclei Kinematics and spectra of planetary nebulae with O VI-sequence nuclei

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...208..127j&link_type=abstract

Astrophysical Journal, vol. 208, Aug. 15, 1976, pt. 1, p. 127-134. Research supported by the Lockheed Independent Research Prog

Astronomy and Astrophysics

Astrophysics

21

Body Kinematics, Fabry-Perot Interferometers, Oxygen Spectra, Planetary Nebulae, Astronomical Spectroscopy, H Alpha Line, Ring Structures, Supernova Remnants

Scientific paper

Spectral features of NGC 5189 and NGC 6905 are tabulated. Fabry-Perot profiles around H alpha and O III lambda 5007 of NGC 5189, NGC 6905, NGC 246, and NGC 1535, are illustrated. The latter planetary nebula is a non-O VI-sequence, comparison object of high excitation. The kinematics of the four planetary nebulae are simply analyzed. Discussion of these data is motivated by the possibility of collisional excitation by high-speed ejecta from broad-lined O VI-sequence nuclei, and by the opportunity to make a comparison with conditions in the supernova remnant or ring nebula, G2.4 + 1.4, which contains an O VI-sequence nucleus of Population I.

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