The Walkaway Star HP Tau/G2: Evidence for a Stellar Merger
Bo Reipurth, J. Bally, P. Friberg, D.M. Faes, C. Briceno, M.S. Connelley, C. Flores, A.M. Cody, H. Zinnecker

TL;DR
This paper presents evidence that the star HP Tau/G2 is the result of a stellar merger, providing insights into stellar evolution, dynamics, and the potential commonality of such events in young stellar objects.
Contribution
It offers the first detailed case study linking a stellar merger to observable properties of a T Tauri star and discusses the dynamical history leading to its formation.
Findings
G2 is a low-mass, rapidly rotating star with signs of a recent merger.
The star's properties match those of FK Com, a merger product.
Stellar mergers may be common and relate to FUor eruptions.
Abstract
HP~Tau/G2 is a luminous, short-period, fast-rotating G-type weak-line T Tauri star with a large radius, an oblate shape with gravity-darkening, little circumstellar material, and centered in a slowly expanding cloud cavity. It is an X-ray source and a variable nonthermal radio source. It forms, together with the late-type T Tauri star KPNO 15, a pair of oppositely directed walkaway stars launched when a multiple system broke apart ~5600 yr ago. Momentum conservation indicates a mass of G2 of only ~0.7 Msun, much lower than the ~1.9 Msun determined from evolutionary models. G2 is virtually a twin of FK Com, the prototype of a class of evolved stars resulting from coalescence of W UMa binaries. We suggest that G2 became a very close and highly eccentric binary during viscous evolution in the protostellar stage and with KPNO 15 formed a triple system, which again was part of a larger…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
