WR 138a

WR 138a is a relatively dim WNL star. Modelling WR 138a's spectrum with PoWR gives a luminosity of around 200,000 L☉ and a temperature of approximately 40,000 K. Using the Stefan-Boltzmann Law the star's radius can be calculated, which turns out at approximately 9.4 R☉.^[3] WR 138a has a very strong stellar wind, typical of Wolf-Rayet stars, and it loses 10^−4.7 M☉ (about 2×10⁻⁵ M_☉) per year because of this stellar wind, which has a terminal velocity of about 700 kilometres per second.^[3] Therefore, the star loses around 1 solar mass every 50,000 years.

WR 138a has a current mass of about 13 M☉, and probably evolved from a star with an initial mass of about 30 M☉, and is about 6.7 million years old. The small size and nearly circular shape of the nebula around WR 138a imply that the stellar wind interacts with the dense ambient medium comoving with the star, which is what shapes the nebula. This consideration suggests that the immediate precursor of WR 138a was a red supergiant (i.e. the star's initial mass is below 40 M☉) and that the WR wind still propagates and ploughs through the high-density region around the star, which is occupied by material shed by the star during its RSG phase.

According to evolution models, stars with initial masses of 25 to 40 M☉ have lifecycles of O → RSG → WN, and the evolution of WR 138a is consistent with the models. Considering average cumulative RSG mass loss values, and velocities, a dynamical age of WR 138a's nebula can be obtained, which turns out at 14,000 years old, which suggests that WR 138a only recently entered the WR phase.^[3]