Fig. 7 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. 7.

Orbital velocities for the primary and secondary around the mass center in NGC 1313 X‐2. A ﹩Z=0.2﹩ Z_⊙ secondary (8.5 M_⊙, 7 R_⊙) and an O7 V secondary (30M_⊙, 9R_⊙) are considered for the system.

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