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High-resolution X-Ray Spectroscopy of the Nova-like Cataclysmic Variable BZ Cam Using Chandra HETG: Diagnosis of the ADAF-like (Advective) Hot Flow

  • Authors: Şölen Balman, Eric M. Schlegel, Patrick Godon, Jeremy J. Drake, Edward M. Sion

Şölen Balman et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 2.

Fits to the joint HETG, HEG, and MEG spectra of BZ Cam. HETG spectra are fit simultaneously with the model, tbabs ×zxipcf×(VNEI+power) on the left and tbabs ×pcfabs×zxipcf×(VNEI) model on the right. The residuals of the fits are displayed in the lower panels in standard deviations (in sigmas).

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