J/ApJ/619/755ivo://CDS.VizieR/J/ApJ/619/755doi:10.26093/cds/vizier.16190755CDSDopita M.A.Groves B.A.Fischera J.Sutherland R.S.Tuffs R.J.,Popescu C.C.Kewley L.J.Reuland M.Leitherer C.2017-06-30T05:48:00Z2007-01-02T09:36:57ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frastronomical-modelsinterstellar-mediumgalaxiesinfrared-sourcesIn this paper, we combine the stellar spectral synthesis code STARBURST99, the nebular modeling code MAPPINGS IIIq, a one-dimensional dynamical evolution model of H II regions around massive clusters of young stars, and a simplified model of synchrotron emissivity to produce purely theoretical self-consistent synthetic spectral energy distributions (SEDs) for (solar metallicity) starbursts lasting ~10^8^yr. These SEDs extend from the Lyman limit to beyond 21cm. We present detailed SED fits to Arp 220 and NGC 6240, and we give the predicted colors for starburst galaxies derived from our models for the IRAS and the Spitzer Space Telescope MIPS and IRAC instruments. Our models reproduce the spread in observed colors of starburst galaxies. Finally, we present absolute calibrations to convert observed fluxes into star formation rates in the UV (GALEX), at optical wavelengths (H), and in the IR (IRAS or Spitzer).2005ApJ...619..755Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/619/755CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/619/755https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/619/755http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/619/755https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/619/755https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/619/755http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/619/755GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/ApJ/619/755/table6Model starburst SEDsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintP/kISM pressurecm**-3.Kphys.pressurefloatFreqFrequencyHzem.freqdoubleLambdaWavelengthumem.wldoublenuFnu1The 1Myr model {nu}f({nu}) (1)mW.m**-2phot.flux.densitydoublenuFnu2The 2Myr model {nu}f({nu}) (1)mW.m**-2phot.flux.densitydoublenuFnu4The 4Myr model {nu}f({nu}) (1)mW.m**-2phot.flux.densitydoublenuFnu8The 8Myr model {nu}f({nu}) (1)mW.m**-2phot.flux.densitydoublenuFnu16The 16Myr model {nu}f({nu}) (1)mW.m**-2phot.flux.densitydoublenuFnu32The 32Myr model {nu}f({nu}) (1)mW.m**-2phot.flux.densitydoublenuFnuLLinear combination model {nu}f({nu}) (1)mW.m**-2phot.flux.densitydoubleFnu1The 1Myr model f({nu}) (2)mW.m**-2.Hz**-1phot.flux.densitydoubleFnu2The 2Myr model f({nu}) (2)mW.m**-2.Hz**-1phot.flux.densitydoubleFnu4The 4Myr model f({nu}) (2)mW.m**-2.Hz**-1phot.flux.densitydoubleFnu8The 8Myr model f({nu}) (2)mW.m**-2.Hz**-1phot.flux.densitydoubleFnu16The 16Myr model f({nu}) (2)mW.m**-2.Hz**-1phot.flux.densitydoubleFnu32The 32Myr model f({nu}) (2)mW.m**-2.Hz**-1phot.flux.densitydoubleFnuLLinear combination model f({nu}) (2)mW.m**-2.Hz**-1phot.flux.densitydoubleJ/ApJ/619/755/table7Galex, IRAS, and Spitzer filter functionsFreqFrequencyHzem.freqdoubleLambdaWavelengthumem.wldoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalex1500AGalex 1500 Angstrom filter transmissionphys.transmission;instr.filterdoubleGalex2300AGalex 2300 Angstrom filter transmissionphys.transmission;instr.filterdoubleIRAS100umIRAS 100 micron filter transmissionphys.transmission;instr.filterfloatIRAS60umIRAS 60 micron filter transmissionphys.transmission;instr.filterfloatIRAS25umIRAS 25 micron filter transmissionphys.transmission;instr.filterfloatIRAS12umIRAS 12 micron filter transmissionphys.transmission;instr.filterfloatIRAC3.5umIRAC 3.5 micron filter transmissionphys.transmission;instr.filterfloatIRAC4.5umIRAC 4.5 micron filter transmissionphys.transmission;instr.filterfloatIRAC5.7umIRAC 5.7 micron filter transmissionphys.transmission;instr.filterfloatIRAC7.9umIRAC 7.9 micron filter transmissionphys.transmission;instr.filterfloatMIPS160umMIPS 160 micron filter transmissionphys.transmission;instr.filterfloatMIPS70umMIPS 70 micron filter transmissionphys.transmission;instr.filterfloatMIPS24umMIPS 24 micron filter transmissionphys.transmission;instr.filterfloatJ/ApJ/619/755/table8Attenuation curve for the models presented in the paperrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLambdaWavelengthumem.wldoubleAttenThe E(Lambda-V)/E(B-V) attenuationphys.absorptiondouble