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The Walkaway Star HP Tau/G2: Evidence for a Stellar Merger

  • Authors: Bo Reipurth, J. Bally, P. Friberg, D. M. Faes, C. Briceño, M. S. Connelley, C. Flores, A. M. Cody, H. Zinnecker

Bo Reipurth et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 12.

A figure illustrating the oblate shape of G2 with gravity darkening. The flattening (Req/Rpol) is ∼1.3, assuming that the mass is 0.7 M, r sini = 3.1 R, v sini = 130 km s−1, and i = 60°. The gravity-darkening exponent is β = 0.16, as derived by F. Espinosa Lara & M. Rieutord (2011). The mass and inclination are the most uncertain parameters. For these parameters, log gpole = 3.40 and log geq = 2.57. This can be compared to the (uncertain) measurement of g ∼ 3.6 (see Section 6.3).

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