A high-resolution study of superficially normal late B spectra

Details A high-resolution study of superficially normal late B spectra A high-resolution study of superficially normal late B spectra

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pasp...92..159c&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 92, Apr.-May 1980, p. 159-164. NSF-supported research.

Astronomy and Astrophysics

Astronomy

22

B Stars, Late Stars, Metallic Stars, Stellar Spectra, A Stars, Hertzsprung-Russell Diagram, High Resolution, M Stars, Manganese, Spectral Resolution

Scientific paper

High-dispersion observations of 13 sharp-lined spectra of late B stars
are intercompared. All stars had MK types and appeared superficially
normal. Two of these objects are clearly related to the manganese stars,
while a third may be a 'hot, hot Am'. The selection effect arising from
the difficulty of detecting mild hot manganese stars is discussed.

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