diff --git a/src/black_holes/EAGLE/black_holes_iact.h b/src/black_holes/EAGLE/black_holes_iact.h index 50fc94677ffdeb9a5109152d56c88aeeb4d1f21b..19a9097605f6053777f1db7b581ab373c0658d83 100644 --- a/src/black_holes/EAGLE/black_holes_iact.h +++ b/src/black_holes/EAGLE/black_holes_iact.h @@ -208,7 +208,7 @@ runner_iact_nonsym_bh_gas_density( /* Minimise separation between the gas particles and the BH. The rays * structs with smaller ids in the ray array will refer to the particles * with smaller distances to the BH. */ - ray_minimise_distance(-pj->rho, bi->rays, arr_size, gas_id, pj->mass); + ray_minimise_distance(pj->rho, bi->rays, arr_size, gas_id, pj->mass); break; } case AGN_random_ngb_model: { diff --git a/src/feedback/EAGLE/feedback_iact.h b/src/feedback/EAGLE/feedback_iact.h index a7dde854088db446203537a71eac1dafcf9841ca..373c6f41d0067d1d7ef8458265935df27a56748e 100644 --- a/src/feedback/EAGLE/feedback_iact.h +++ b/src/feedback/EAGLE/feedback_iact.h @@ -140,7 +140,7 @@ runner_iact_nonsym_feedback_density(const float r2, const float *dx, /* Minimise separation between the gas particles and the star. The rays * structs with smaller ids in the ray array will refer to the particles * with smaller distances to the star. */ - ray_minimise_distance(-rho, si->feedback_data.SNII_rays, arr_size, pj->id, + ray_minimise_distance(rho, si->feedback_data.SNII_rays, arr_size, pj->id, pj->mass); break; }