Ultraviolet observations of the X-ray sources in the Eta Carinae nebula

Details Ultraviolet observations of the X-ray sources in the Eta Carinae nebula Ultraviolet observations of the X-ray sources in the Eta Carinae nebula

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssrv...30..235v&link_type=abstract

(European Space Agency, ESLAB Symposium on X-ray Astronomy, 15th, Amsterdam, Netherlands, June 22-26, 1981.) Space Science Revie

Astronomy and Astrophysics

Astronomy

9

Astronomical Spectroscopy, Iue, Nebulae, Ultraviolet Astronomy, X Ray Sources, Absorption Spectra, Satellite Observation, Spectral Resolution, Spectrum Analysis, Stellar Envelopes, Stellar Mass Ejection, Stellar Spectra

Scientific paper

Eta Car is surrounded by a dense nebula ejected during the last 150 years. The Einstein satellite recently detected intense X-ray emission from Eta Car and its nebula indicating the existence of efficient gas heating processes. Ultraviolet observations with IUE confirmed the presence of hot gas in the condensation S of the nebula and in Eta Car. Possible interpretations of the results are discussed.

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