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The Eclipsing Novalike Cataclysmic Variable CRTS SSS100505 J093417-174421

  • Authors: Raymundo Baptista, Albert Bruch, Raimundo Lopes de Oliveira, Cláudia V. Rodrigues, Alexandre S. Oliveira, Isabel J. Lima

Raymundo Baptista et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 4.

(a) Dependency on orbital phase of the maximum intensity derived from the asymmetric component of the V-band (black) and I-band (red) eclipse maps. Intensities are plotted on an arbitrary scale; arms 1 and 2 are labeled, and horizontal tick marks indicate the phases of maxima of the double-wave orbital modulation. Dotted lines show the uncertainties at the 1σ limit. Vertical dashed lines mark the 1σ range of values for the phase of lowest intensity, ﹩{\phi }_{1}({I}_{{\rm{\min }}})﹩ (see text). (b) Corresponding radius of maximum intensity in units of RL1. Horizontal dashed lines mark the circularization radius (Rcirc = 0.208 RL1) and the outer disk radius (RV = 0.36 RL1 in the V band and RI = 0.54 RL1 in the I band).

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