Spectrophotometry in the upper Scorpius region

Details Spectrophotometry in the upper Scorpius region Spectrophotometry in the upper Scorpius region

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..348g&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, June-July 1979, p. 348-355.

Astronomy and Astrophysics

Astronomy

Scorpius Constellation, Spectral Energy Distribution, Spectral Line Width, Stellar Spectra, Stellar Spectrophotometry, Balmer Series, H Beta Line, H Gamma Line, Stellar Luminosity, Tables (Data), Ubv Spectra

Scientific paper

The low dispersion spectrophotometric measures of 29 stars in the upper Scorpius region, made from 1964 to 1969 with an old-type spectrum scanner, employing a 91 cm telescope with a 60 A slit, are examined. Equivalent widths of H-beta, H-gamma, and H-delta are measured along with the size of the Balmer discontinuity, the gradients in the ultraviolet and the blue-green-yellow parts of the spectrum. The results of the intensity distributions, the spectral intensity distributions, and some measured quantities are presented in tabulated form.

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