Multiplex imagery of the infrared core of Eta Carinae

Details Multiplex imagery of the infrared core of Eta Carinae Multiplex imagery of the infrared core of Eta Carinae

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...146l...1b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 146, no. 1, May 1985, p. L1, L2.

Astronomy and Astrophysics

Astrophysics

13

Infrared Stars, Stellar Cores, Stellar Envelopes, Stellar Mass Ejection, Condensation, Cosmic Dust, Image Processing, Stellar Winds

Scientific paper

Infrared observation of Eta Car at the 3.6 m ESO telescope with the Multiplex coding technique, have revealed the presence of a compact core with a full width at 1/e intensity of ≡0arcsec.13 at 1.25 to 3.7 μm, and 0arcsec.23 at 4.8 μm. This is most likely the inner layer of the dust envelope where the grains start to condense from the intense stellar wind.

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