Molecular hydrogen ion /H2+/ absorption in planetary nebulae

Details Molecular hydrogen ion /H2+/ absorption in planetary nebulae Molecular hydrogen ion /H2+/ absorption in planetary nebulae

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86..881f&link_type=abstract

Astronomical Journal, vol. 86, June 1981, p. 881-884.

Astronomy and Astrophysics

Astronomy

5

Absorption Spectra, Astronomical Spectroscopy, Hydrogen Ions, Molecular Ions, Planetary Nebulae, Iue, O Stars, Positive Ions, Wavelengths

Scientific paper

Several IUE spectra of planetary nebulae show an absorption feature
shortward of 1500 A which is believed to be due to H2(+). The nebulae
are excited by stars of spectral type O3-O7 or continuum, and all but
one have double-shell structure.

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