コード例 #1
0
dflist,d  = read_in_datafiles('file20.txt')

dname = sorted(d.values())

dflist = stars_outside_2HMR(dflist,dname)


#%% print the count the number of stars outside 2xHMR in a snapshot....

print (dname[5])
print (dflist[5].loc[10]['escaped'].value_counts())

#%%

dflist = velocity_elements(dflist,dname)

for n in range(20):
    dflist[n]['3D-vel'] = (np.sqrt(dflist[n]['velx']**2.+dflist[n]['vely']**2.+dflist[n]['velz']**2.))
    dflist[n]['3D-veldist'] = (np.sqrt(dflist[n]['xvel']**2.+dflist[n]['yvel']**2.+dflist[n]['zvel']**2.))
    dflist[n]['PM-vel'] = (np.sqrt(dflist[n]['velx']**2.+dflist[n]['vely']**2.))
    dflist[n]['PM-veldist'] = (np.sqrt(dflist[n]['xvel']**2.+dflist[n]['yvel']**2.))
    dflist[n].ESC = (dflist[n].loc[dflist[n]['escaped'] == True])  
    
ESClist = [dflist[0].ESC, dflist[1].ESC, dflist[2].ESC, dflist[3].ESC, dflist[4].ESC,dflist[5].ESC,dflist[6].ESC,dflist[7].ESC,dflist[8].ESC,dflist[9].ESC,dflist[10].ESC, \
          dflist[11].ESC, dflist[12].ESC, dflist[13].ESC, dflist[14].ESC, dflist[15].ESC, dflist[16].ESC, dflist[17].ESC, dflist[18].ESC,dflist[19].ESC]
 
ESC = pd.concat(ESClist)


#%% plots umulative velocity distribution for unbound stars at 5 Myr as PM-velocity and 3D-velocity
コード例 #2
0
#!/usr/bin/env python3
# -*- coding: utf-8 -*-
"""
Created on Fri May 18 13:48:50 2018

@author: php17cs
"""

import numpy as np
from function_file import read_in_any_datafiles, velocity_elements, plots_legend

#reads in the .dat files from an inputfile list
dflist, dname, nlines = read_in_any_datafiles('file.txt')

#calculates the velocity (distance travelled/snapshot length
dflist = velocity_elements(dflist, dname, nlines)

#creates the legend for for plots of single simulations
legend = plots_legend(dname)

j = 50
velocity = 'PM-velxy'

dflist_mean = np.empty(1000)

for line in range(1000):
    dflist_sumlist = []
    for n in range(nlines):
        dflist_sumlist.append(
            (dflist[n].loc[j].sort_values(velocity)[velocity]).iloc[line])
    dflist_mean[line] = (np.mean(dflist_sumlist))
コード例 #3
0
import pandas as pd
import numpy as np
import matplotlib.pyplot as plt
from matplotlib.ticker import AutoMinorLocator
#import F_COD_Radius_Nstars as CODRN  #turn this on, if COD-correcion is required.
from function_file import read_in_any_datafiles, velocity_elements, energy_stars, stars_in_outside_2HMR

dflist, dname, nlines = read_in_any_datafiles(
    'file.txt')  #this reads in the .dat files from an inputfile list

dflist = energy_stars(
    dflist, dname, nlines
)  #this calculates the energy of each star in each snapshot an simulation and adds this in a column
dflist = velocity_elements(
    dflist, dname, nlines
)  #this calculates the velocity by using the distance travelled between each snapshot and divides it by snapshot length - this is an alternative to the provided velocities from the simulation
dflist = stars_in_outside_2HMR(
    dflist, dname, nlines
)  # this calculates the half-mass radius based on centre of density corrected locations and then adds a column identifying if the stars are inside or outside 2*HMR

# different velocity distributions are calculated, e.g. 3D and PM for the original velocity data velx - velz and the velocities calculated by using the distance travelled between each snapshot.
#both are expressed in km/s
#%% this cell produces dataframes for each simulation containing the unbound/escaped stars,
# this cell also creates dataframes for each simulation containing the high-mass and low-mass unbound and escaped stars.

dflistUB = []
dflistESC = []
dflistHMUB = []
dflistHMESC = []
dflistHMall = []