def calc_ne(mass, size): nh = nhs[args.iden] logQ = logQ_interp(mass) stro = koo.calcStromgrenRadius(logQ, nh) radius = 0.5 * size * PC2CM ne = nh * (stro / radius)**(1.5) return ne
def calcStagnationTime(logQ, nh): ci = koo.soundSpeed(8000.0, 0.5) co = koo.soundSpeed(10.0, 1.0) cico = ci / co RS = koo.calcStromgrenRadius(logQ, nh) ts = RS / ci return (4.0 / 7.0) * ((3.0 / 4.0)**0.5) * (((4.0 / 3.0)**(7.0 / 6.0)) * (cico**(7.0 / 3.0)) - 1.0) * ts
casa_ang_size = np.zeros(nstars, dtype=float) tot_flux = np.zeros(nstars, dtype=float) casa_tot_flux = np.zeros(nstars, dtype=float) casa_peak_flux = np.zeros(nstars, dtype=float) g_long = star_data[:,15] g_lat = star_data[:,16] for i in range(1, nstars + 1): t = age[i - 1] * 1000.0 * YR2S m = mcur[i - 1] nh = nhs[args.iden] logQ = float(logQ_interp(m)) #dsun = d_sun[i - 1] * 1000.0 * PC2CM dsun = 5.0 * 1000.0 * PC2CM stro = koo.calcStromgrenRadius(logQ, nh) raga = koo.calcSpitzerRadius(logQ, nh, t) stag = koo.calcStagnationRadius(logQ, nh) #radius = np.minimum(raga, stag) radius = raga angsize_rad = (2.0 * radius / dsun) angsize_as = angsize_rad * 60.0 * 60.0 * 180.0 / math.pi ne = nh * (stro / radius)**(1.5) T = 8000.0 f = 5.0e9 tau = calcTau(T, f, ne, logQ) B = calcPlanck2(T, f) * 1.0e26 S = B * (1.0 - math.exp(-tau)) F = S * (0.5 * angsize_rad)**2 * 1000
r = "{:4.2f}".format(rstar[j])
l = "{:4.2f}".format(logL[j])
q = "{:4.2f}".format(logQ[j])
ed = "{:4.2e}".format(0.5 * mdot[j] * vinf[j] * vinf[j]) # erg.s-1
md = "{:8.2e}".format(mdot[j] / 6.341958397e25) # [Msun.yr-1]
v = "{:8.2e}".format(vinf[j] / 100000.0) # [km.s-1]
print m + " & " + t + " & " + r + " & " + l + " & " + q + " & " + ed + " & " + md \
+ " & " + v + " \\\\"
for i in range(len(den)):
for j in range(len(mass)):
index = 9*i + j
m = "{:3d}".format(int(mass[j]))
d = "{:8.2e}".format(den[i])
ysc = "{:4.3f}".format(koo.calcStromgrenRadius(logQ[j], den[i]) / cloud_dist)
nx = str(nxs[index])
ny = str(nys[index])
nxny = "{($" + nx + "$,$" + ny + "$)}"
sizex = "{:3.2f}".format(sizexs[index] / 3.09e18)
r_inj = 10.0 * sizexs[index] / nxs[index]
lcrit = "{:4.3e}".format(critL2(r_inj, vinf[j]))
tstart = "{:4.3f}".format(koo.calcStartTime(mdot[j], vinf[j], mh*den[i], 8000.0, 0.5, r_inj) * S2YR / 1000.0)
tcoolval = coolTime(mp1_data.central_pressures[index], mp1_data.central_densities[index]) * S2YR / 1000.0
tcool = "{:4.3e}".format(tcoolval)
texitval = exitTime(r_inj, vinf[j]) * S2YR / 1000.0
texit = "{:4.3f}".format(texitval)
R_inj = "{:4.3f}".format(r_inj * CM2PC)
ri = "{:8d}".format((int)(-tcoolval / texitval))
print m + " & " + d + " & " + nx + " & " + ny + " & " + sizex + " & " + ysc + " & " + R_inj + " & " + tstart + " & " + tcool + " \\\\"
def printPaperTable(r, t, b, isWind, isMVD):
T = 8000.0
mu = 0.5
diststr = "D_\\mathrm{s}" if isWind else "D_\\mathrm{i}"
numstr = "4" if isWind else "4"
for row in range(9):
mass = massList[row]
mdot = mdotList[row]
vinf = vinfList[row]
logQ = logQList[row]
nhs_hii = mvd_iden if isMVD else mvt_iden
times = mvd_times if isMVD else mvt_times
nhs_init = mvd_nhs if isMVD else mvt_nhs
inj = mvd_inj if isMVD else mvt_inj
tableline = "\multirow{" + numstr + "}{*}{\\num{" + str(mass) + "}} & {$" + diststr + "(0)$}"
for col in range(5):
tableline = tableline + " & "
tableline = tableline + str(t[col][row])
print tableline + " \\\\"
tableline = "& {$" + diststr + "(\\frac{\\pi}{2})$}"
for col in range(5):
tableline = tableline + " & "
tableline = tableline + str(r[col][row])
print tableline + " \\\\"
tableline = "& {$" + diststr + "(\\pi)$}"
for col in range(5):
tableline = tableline + " & "
tableline = tableline + str(b[col][row])
print tableline + " \\\\"
if isWind:
tableline = "& {$R_\\mathrm{P}$}"
for col in range(5):
tableline = tableline + " & "
R = koo.calcFinalRadiusRB(mdot, vinf, mh*nhs_hii[col][row], T, mu) * CM2PC
tableline = tableline + str(R)
print tableline + " \\\\"
else:
tableline = "& {$R_\\mathrm{raga-1}$}"
for col in range(5):
tableline = tableline + " & "
R = koo.calcStromgrenRadius(logQ, nhs_init[col])
#R = max(R, inj[col][row] / CM2PC)
R = koo.calcSpitzerRadius2(R, times[col]*YR2S)*CM2PC
R = koo.calcExactIF(300.0, T, 1.0, mu, nhs_init[col], 10.0**logQ,
times[col] * YR2S, is_spitzer=True) * CM2PC
tableline = tableline + str(R)
print tableline + " \\\\"
#tableline = "& {$R_\\mathrm{stag}$}"
#for col in range(5):
# tableline = tableline + " & "
# R = koo.calcStromgrenRadius(logQ, nhs_init[col])
# #R = max(R, inj[col][row] / CM2PC)
# R = koo.calcStagnationRadius2(R) * CM2PC
# tableline = tableline + str(R)
#print tableline + " \\\\"
if row != 8:
print "& & & & & & \\\\"
#mvd_iden.append([610.0, 480.0, 650.0, 900.0, 1300.0, 1800.0, 2200.0, 2400.0, 2700.0]) #mvd_iden.append([800.0, 900.0, 1000.0, 1400.0, 2100.0, 2500.0, 3000.0, 5000.0, 5000.0]) #mvd_iden.append([2000.0, 2200.0, 2200.0, 2400.0, 3000.0, 4500.0, 5500.0, 7000.0, 12000.0]) #mvt_iden = [] #mvt_iden.append([520.0, 620.0, 1000.0, 1700.0, 2600.0, 4500.0, 6500.0, 9000.0, 12000.0]) #mvt_iden.append([620.0, 520.0, 750.0, 1000.0, 1600.0, 2400.0, 2500.0, 5000.0, 8000.0]) #mvt_iden.append([580.0, 520.0, 600.0, 800.0, 1400.0, 1800.0, 1900.0, 2500.0, 3000.0]) #mvt_iden.append([520.0, 550.0, 550.0, 700.0, 1100.0, 1300.0, 1500.0, 1700.0, 1800.0]) #mvt_iden.append([520.0, 540.0, 520.0, 620.0, 850.0, 1200.0, 1300.0, 1400.0, 1500.0]) mvd_iden = [] for i in range(5): arr = [] for j in range(9): R_strom = koo.calcStromgrenRadius(logQList[j], mvd_nhs[i]) * CM2PC #R_strom = max(R_strom, mvd_inj[i][j]) arr.append(mvd_nhs[i] * math.pow(R_strom / mvd_IF_r[i][j], 1.5)) mvd_iden.append(arr) mvt_iden = [] for i in range(5): arr = [] for j in range(9): R_strom = koo.calcStromgrenRadius(logQList[j], mvt_nhs[i]) * CM2PC #R_strom = max(R_strom, mvt_inj[i][j]) arr.append(mvt_nhs[i] * math.pow(R_strom / mvt_IF_r[i][j], 1.5)) mvt_iden.append(arr) if print_sizes:
