diff --git a/COSMIC/COSMIC_v3_emission.py b/COSMIC/COSMIC_v3_emission.py deleted file mode 100644 index 6a59ebe..0000000 --- a/COSMIC/COSMIC_v3_emission.py +++ /dev/null @@ -1,53 +0,0 @@ -""" -* COSMIC - EMISSION -* Version 3 -@ Yaƫl Moussouni -@ Unistra, P&E, MSc1-MoFP -@ Observatory of Strasbourg (Intern) -""" - -import numpy as np -import amuse.units.units as u - -def rotation(stars, params): - N = params["N_stars"] + np.int32(np.round(params["N_stars"] * params["binary_fraction"])) - stars.X_v = np.random.uniform(0, 10, N) | u.km * u.s**(-1) - p = np.random.uniform(0, 1, N) - stars.X_vsini = stars.X_v * np.sqrt(2*p-p**2) - return stars - -def X_emission(stars, params): - for i in range(len(stars)): - if stars[i].temperature.value_in(u.K) > 7300: # O B A - stars[i].X_luminosity = params["X_coefficient_OBA"] * stars[i].luminosity.in_(u.erg * u.s**(-1)) - elif stars[i].temperature.value_in(u.K) < 6000: # G K M - stars[i].X_luminosity = params["X_coefficient_GKM"] * (stars[i].X_vsini.value_in(u.km * u.s**(-1)))**(1.9) | u.erg * u.s**(-1) - else: # F - stars[i].X_luminosity = 0 | u.erg * u.s**(-1) - return stars - -def plasma_temperature(stars, params): - for i in range(len(stars)): - if stars[i].temperature.value_in(u.K) > 7300 : # O B A - if stars[i].age.value_in(u.Myr) < 150: # young - stars[i].X_temperature_0 = 0.6 | u.kilo(u.eV) - stars[i].X_temperature_1 = 0.0 | u.kilo(u.eV) - else: # old - stars[i].X_temperature_0 = 0.5 | u.kilo(u.eV) - stars[i].X_temperature_1 = 0.0 | u.kilo(u.eV) - elif stars[i].temperature.value_in(u.K) < 6000: # G K M - if stars[i].age.value_in(u.Myr) < 150: # young - stars[i].X_temperature_0 = 0.4 | u.kilo(u.eV) - stars[i].X_temperature_1 = 1.0 | u.kilo(u.eV) - else: # old - stars[i].X_temperature_0 = 0.2 | u.kilo(u.eV) - stars[i].X_temperature_1 = 0.8 | u.kilo(u.eV) - else: # F - if stars[i].age.value_in(u.Myr) < 150: # young - stars[i].X_temperature_0 = 0.6 | u.kilo(u.eV) - stars[i].X_temperature_1 = 0.0 | u.kilo(u.eV) - else: # old - stars[i].X_temperature_0 = 0.5 | u.kilo(u.eV) - stars[i].X_temperature_1 = 0.0 | u.kilo(u.eV) - - return stars