Classification spectra of Sanduleak and Stephenson emission-line star

Details Classification spectra of Sanduleak and Stephenson emission-line star Classification spectra of Sanduleak and Stephenson emission-line star

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184..601a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 184, Sept. 1978, p. 601-610.

Other

50

Astronomical Spectroscopy, Emission Spectra, Stellar Spectra, Balmer Series, Classifications, H Lines, Line Spectra, Spectrum Analysis, Tables (Data), Wolf-Rayet Stars

Scientific paper

Low-dispersion slit spectra of 89 emission-line stars are described; these stars were originally located and classified by Sanduleak and Stephenson in an objective-prism survey. The new data broadly confirm the classification scheme adopted by Sanduleak and Stephenson. In particular most of the large number of symbiotic stars they classified have been confirmed and others found. Many of these contain strong, broad emission bands in their red spectra. Two new Wolf-Rayet stars, one new planetary nebula and two new bipolar reflection nebulae involving hidden emission-line stars have been found.

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