Ali A., Harries T. J., Douglas T. A., 2018, MNRAS, 477, 5422 (doi:10.1093/mnras/sty1001) ionrp (ionization + radiation pressure) notes - ???? indicates dump number (0076-0392) - radiation initiated from 0076 - dumps separated by 0.5e4 yr - ### indicates source number (001-029, descending in initial mass) ---------------- grids????-????.zip (grouped in sets of 5) - dump_????.grid (torus grid file) dumpvtu????-????.zip (grouped in sets of 10) - dump_????.vtu (vtk files for grid, e.g. density, temperature, etc.) nbody.zip (all) - nbody_????.vtk (vtk files for sources) source.zip (all) - source_????.dat (torus source file) logs.zip - parameters.dat (torus parameters file) - log (torus print statements) radial.zip nb: columns are (1) r (2) rho (3) u (4) rhoe (5) p (6) phi_stars (7) phi_gas (8) kappa*Flux (9) radmom (10) radpressure (11) temperature (12) tdust - radial+X????.dat (cell values from grid centre to boundary, advancing in +x direction) - radial+Y????.dat (+y direction) - radial+Z????.dat (+z direction) - radial+XYZ????.dat (+xyz direction) columnz.zip - columnz_????.fits (fits files showing column density in g/cm2) sourceinfo.zip - sourceinfo_###.fits (info for star number ###, e.g. mass, radius, luminosity, position) synthetic observations (t = colatitude theta, p = azimuth phi in degrees) - halpha.zip - sii6731.zip - oiii5007.zip - freefree.zip - dustimages.zip - as well as observations, also includes... --- ????_avgtdust_*.fits (mean dust temp weighted by mass, or no weighting) --- ????_normvarianceTdust_*.fits (variance normalised by mean value, for different weights) analysis.zip - plotting scripts - starburst.py (star positions and column density at starburst) - opacity.py & albedo01.dat (opacity vs wavelength) - makeplot.py (bulk grid properties) - multidensityfits.py (column density snapshots) - multirgb.py (HST plot) - densitypdfSinglePlot.py (column density PDFs) - globaltempplot.py (T vs time) - globalneplot.py (ne vs time) - habingplot.py (G0 around star 1 vs time) - habingplot2.py (G0 around star 25 vs time) - luminosityhalpha.py (Halpha luminosity/extinction vs time) - nlyman.py (NLy vs time) - bbratio.py (450 and 850 um plots) - tables of data - tableoftotals.dat (total of variables on grid, eg mass) - valuesOnGrid.dat (more totals) - tableofnlyman.dat (NLy from integrated stellar spectra) - estimatedLymanFlux.dat (NLy from recombination rate - RHS of eq. 30, assuming case A, case B, Rubin1968 coefficients) - avgtempGlobalRms*.dat (average/stddev of T, ne, for different weights) - averageHabingFlux.dat (G0 around star 1 in Habing units) - averageHabingFlux_allStars.dat (G0 around each star in Habing units)