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W. Hartmann

1 paper here

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astro-ph2004

A New View of the Supersoft X-Ray Source Cal 87 Observed with XMM-Newton

Marina Orio, Ken Ebisawa, John Heise +1

Cal 87 was observed with XMM-Newton in April of 2003. The source shows a rich emission line spectrum, where lines can be identified if they are red-shifted by 700-1200 km/s. These…

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