Figure 3 from X-Ray Emission and Corona of the Young Intermediate-Mass Binary θ1 Ori E

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X-Ray Emission and Corona of the Young Intermediate-Mass Binary θ1 Ori E

Authors: David P. Huenemoerder, Norbert S. Schulz, Paola Testa, Anthony Kesich, and Claude R. Canizares

HUENEMOERDER et al. 2009 The Astrophysical Journal 707 942.

Provider: AAS Journals

Caption: Figure 3.

Reconstructed emission measure, for a distance of 450 pc and N _H = 2 × 10 ²¹ cm ^-2. The upper and lower gray boundaries are 1σ (logarithmic) statistical uncertainties from Monte Carlo iterations in which the measured fluxes were perturbed randomly according to their measurement uncertainties. The integrated emission measure is 1.2 × 10 ⁵⁵ cm ^-3.

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