diff --git a/src/entropy_floor/none/entropy_floor.h b/src/entropy_floor/none/entropy_floor.h index cc1569d7a06389af1f523da3878f052ce493d07f..6ce5319c8c76cf8f9e6dc1716f383452d7cce7d6 100644 --- a/src/entropy_floor/none/entropy_floor.h +++ b/src/entropy_floor/none/entropy_floor.h @@ -56,14 +56,14 @@ static INLINE float entropy_floor( * @brief Compute the temperature from the entropy floor for a given #part * * Simply return 0 (no floor). - * + * * @param p The #part. * @param cosmo The cosmological model. * @param props The properties of the entropy floor. */ static INLINE float entropy_floor_temperature( const struct part *p, const struct cosmology *cosmo, - const struct entropy_floor_properties *props){ + const struct entropy_floor_properties *props) { return 0.f; } diff --git a/src/runner.c b/src/runner.c index a3b91e1e8b250f1ee22297565bc8b78efcfef85d..984bce52cfc750f984e30d50e93825d659964769 100644 --- a/src/runner.c +++ b/src/runner.c @@ -605,7 +605,8 @@ void runner_do_star_formation(struct runner *r, struct cell *c, int timer) { /* Is this particle star forming? */ if (star_formation_is_star_forming(p, xp, sf_props, phys_const, cosmo, - hydro_props, us, cooling, entropy_floor)) { + hydro_props, us, cooling, + entropy_floor)) { /* Time-step size for this particle */ double dt_star; diff --git a/src/star_formation/EAGLE/star_formation.h b/src/star_formation/EAGLE/star_formation.h index 92ddcc1c5e3ba34c1f51b94e71a562948a583fce..0fc044170b2ed46caba1975078114f5c51f51e71 100644 --- a/src/star_formation/EAGLE/star_formation.h +++ b/src/star_formation/EAGLE/star_formation.h @@ -246,7 +246,8 @@ INLINE static int star_formation_is_star_forming( us, cosmo, cooling, p, xp); /* Temperature on the equation of state */ - const double temperature_eos = entropy_floor_temperature(p, cosmo, entropy_floor); + const double temperature_eos = + entropy_floor_temperature(p, cosmo, entropy_floor); /* Check the Scahye & Dalla Vecchia 2012 EOS-based temperature critrion */ return (temperature <