The hydrogen-line-strength variation in the AP star HD 184905

Details The hydrogen-line-strength variation in the AP star HD 184905 The hydrogen-line-strength variation in the AP star HD 184905

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978jrasc..72..194r&link_type=abstract

Journal of the Royal Astronomical Society of Canada, vol. 72, Aug. 1978, p. 194-197. Research supported by Brandon University.

Astronomy and Astrophysics

Astronomy

A Stars, H Lines, Magnetic Stars, Stellar Spectra, Astronomical Spectroscopy, H Gamma Line, Spectral Line Width, Variability

Scientific paper

Observations of the hydrogen-line strengths for the Ap star HD 184905 are reported and compared with those given by Kumaigorodskaya and Chunakova (1975). The claim by these authors that all the hydrogen lines exhibit strong variability is questioned in light of the present observations. In particular, their claim that the cores of the hydrogen lines vary more than the wings appears to be in error.

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