Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-01-12
Astronomy and Astrophysics
Astrophysics
6 pages, 6 figures, accepted by ApJ
Scientific paper
10.1086/320961
Sub-arcsecond resolution Chandra observations of Eta Carinae reveal a 40 arcsec X 70 arcsec ring or partial shell of X-ray emission surrounding an unresolved, bright, central source. The spectrum of the central source is strongly absorbed and can be fit with a high-temperature thermal continuum and emission lines. The surrounding shell is well outside the optical/IR bipolar nebula and is coincident with the Outer Shell of Eta Carinae. The X-ray spectrum of the Shell is much softer than that of the central source. The X-ray Shell is irregular and only correlates well with optical features where a bright X-ray knot coincides with a bright feature of the Outer Shell. Implications for the binary model of the central source are discussed.
Butt Yousaf M.
Corcoran Marj
Karovska Magarita
Schlegel Prestwich. E. A. M.
Seward Frederick D.
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