Ultraviolet variations of epsilon UMa

Details Ultraviolet variations of epsilon UMa Ultraviolet variations of epsilon UMa

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975aj.....80..137m&link_type=abstract

Astronomical Journal, vol. 80, Feb. 1975, p. 137-139.

Astronomy and Astrophysics

Astronomy

16

A Stars, Abundance, Spaceborne Astronomy, Stellar Spectrophotometry, Ultraviolet Absorption, Variable Stars, Absorption Spectra, Light Curve, Line Spectra, Metals, Oao 2, Satellite Observation

Scientific paper

OAO-2 spectrometer observations of the Ap variable epsilon UMa indicate
that the photometric variations are due to variable ultraviolet
absorption from apparently overabundant metals. These data also point
out the presence of a secondary maximum of the Fe-group elements,
notably Cr, that has not been reported.

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