Ultraviolet photometry of Eta Carinae and its interpretation

Details Ultraviolet photometry of Eta Carinae and its interpretation Ultraviolet photometry of Eta Carinae and its interpretation

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....47..443p&link_type=abstract

Astronomy and Astrophysics, vol. 47, no. 3, Mar. 1976, p. 443-448.

Astronomy and Astrophysics

Astrophysics

24

Astronomical Photometry, Infrared Radiation, Interstellar Extinction, Stellar Spectra, Ultraviolet Photometry, H Lines, Hydrogen Clouds, Interstellar Matter, Nebulae, Stellar Luminosity, Stellar Spectrophotometry

Scientific paper

Measurements of Eta Carinae in the ultraviolet are reported and used to determine the extinction. It is concluded that the foreground material will produce the observed extinction and that there is no need to introduce anomalous additional extinction, as has been argued by previous authors. The consequences of this for the infrared radiation are discussed along with the intrinsic properties of Eta Carinae

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