Fig. 6 from Optical Studies of the Ultraluminous X‐Ray Source NGC 1313 X‐2

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Optical Studies of the Ultraluminous X‐Ray Source NGC 1313 X‐2

Authors: Ji-Feng Liu, Joel Bregman, Jon Miller, and Philip Kaaret

Liu et al. 2007 The Astrophysical Journal 661 165.

Provider: AAS Journals

Caption: Fig. 6.

Predicted periods for different primary masses for a ﹩Z=0.2﹩ Z_⊙ secondary (8.5 M_⊙, 7 R_⊙) and for an O7 V secondary (30 M_⊙, 9 R_⊙) with solar metallicity. The periods are calculated using the Roche lobe sizes ﹩f( q) ﹩ as tabulated by Kopal, and the analytic approximations by Paczyński and Eggleton.

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