Description of output files from population synthesis models ============================================================ Reference: Schaerer D., Vacca W.D., 1998, ApJ, 497, 168 "New Models for Wolf-Rayet and O Star Populations in Young Starbursts" - Last update on June 18, 1999: Removed constant SF models. For requests contact schaerer@obs-mip.fr - Updated on July 6, 1998 [Version 2.32 (pop_iso_232), July 1998 After correction of normalisation bug of WR atmospheres] ================================================================== Daniel Schaerer e-mail: schaerer@obs-mip.fr Observatoire Midi-Pyrenees phone: (+33) 5 61 33 2929 14, Av. E. Belin direct: (+33) 5 61 33 2898 F-31400 Toulouse fax: (+33) 5 61 33 2840 France http://www.obs-mip.fr/omp/astro/people/schaerer ================================================================== 1) FILES: ========= General nomenclature of filenames: ezzz_imf_mup_sfh.n Where: e Indicates high mass-loss tracks zzz Metallicity (e.g. 020 for Z=0.020) imf Slope of IMF ( 235 alpha=2.35=Salpeter) mup upper mass cut-off of IMF ( 120 120 Msun) sfh code for starformation history: - isb instantaneous burst - dt1 extendend burst of duration 1 Myr - dt2... " " " " 2 " - cs1 constant star formation (ages 0-10 Myr) - cs2 constant star formation (ages 0-100 Myr) n number of output file: - 20 Main output file (--> results in SV98) - 21 Output file for WR lines (--> results in SV98) - 23 Colors of integrated population Each file contains a header including detailed information about all the adopted input parameters, the content of the files and the output units used. 2) DESCRIPTION OF FILE CONTENT: =============================== File *.20 (main output): ~~~~~~~~~~~~~~~~~~~~~~~~ Lines 1-15: HEADER with summary of the input parameters. Lines 16-end: ------------------------------ column content ------------------------------ 1 log(age) [yr] 2 Mbol [mag] 3 log(Q_0) [s^-1] 4 log(Q_1) [s^-1] 5 log(Q_2) [s^-1] 6 # O-stars 7 WR/(WR+O) 8 WR/O 9 WNL = WNL/(WR+O) 10 WNE = WNE/(WR+O) 11 WC = WC /(WR+O) 12 H_beta EW [A] 13 " luminosity [erg s^-1] 14 HeI 4471 EW [A] CAUTION: Saturation effect ! 15 " luminosity [H_beta] 16 nebular HeII 4686 EW [A] 17 " luminosity [H_beta] 18 WR bump (CIII/IV 4650 + HeII 4686) EW [A] <--- WARNING: 19 " luminosity [H_beta] <--- using line flux 20 CIV-WR EW [A] <--- calibration of 21 " luminosity [H_beta] <--- Smith (1991). 22 Balmer jump [magnitudes] 23 log(Q_H2) [s^-1] <-- for internal use only (not documented) ! File *.21 (WR output): ~~~~~~~~~~~~~~~~~~~~~~~~ Lines 1-15: HEADER with summary of the input parameters. Lines 16-end: ------------------------------ column content ------------------------------ 1 log(age) [yr] 2 average WNL subtype <-- for internal use only (not documented) ! 3 average WC subtype 4 H_alpha EW [A] 5 " luminosity [H_beta] 6 H_beta EW [A] 7 " luminosity [erg s^-1] 8 He1640 EW [A] 9 " luminosity [H_beta] 10 N_4640 EW [A] 11 " luminosity [H_beta] 12 C_4650 EW [A] 13 " luminosity [H_beta] 14 He4686 EW [A] 15 " luminosity [H_beta] 16 H_4861 EW [A] 17 " luminosity [H_beta] 18 C_5696 EW [A] 19 " luminosity [H_beta] 20 C_5808 EW [A] 21 " luminosity [H_beta] 22 H_6560 EW [A] 23 " luminosity [H_beta] File *.23 (photometry): ~~~~~~~~~~~~~~~~~~~~~~~~ Broad-band colors of stellar population. The colors include the nebular continuous emission, but neglects the contribution of all nebular and stellar emission lines. The filter response curves and calibration of Leitherer & Heckman (1995, ApJS, 96, 9) are used. Lines 1-15: HEADER with summary of the input parameters. Lines 16-end: ------------------------------ column content ------------------------------ 1 log(age) [yr] 2 (1300-V) 3 (210-V) 4 (U-B) 5 (B-V) 6 (V-R) 7 (V-I) 8 (V-J) 9 (V-H) 10 (V-K) 11 (V-L) 12 M_V 13 M_B 14 M_BOL Files *.tar: ~~~~~~~~~~~~ Tar-files including all of the above described files.