J/MNRAS/469/3125ivo://CDS.VizieR/J/MNRAS/469/3125doi:10.26093/cds/vizier.74693125CDSContini M.2024-08-17T20:19:16Z2020-05-14T08:04:38ZCDS support team

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

cds-question@unistra.frgamma-ray-astronomygamma-ray-burstssupernovaechemical-abundancesThe distribution of the N/O element abundance ratios calculated by the detailed modelling of different galaxy spectra at z<4 is investigated. Supernova (SN) and long gamma-ray-burst (LGRB) host galaxies cover different redshift domains. N/O ratios in SN hosts increase due to secondary N production towards low z (0.01) accompanying the growing trend of active galaxies [active galactic nucleus (AGN), low-ionization nuclear emission-line region (LINER)]. N/O ratios in LGRB hosts decrease rapidly between z>1 and z~0.1 following the N/H trend and reach the characteristic N/O ratios calculated for the H II regions in local and nearby galaxies. The few short-period gamma-ray-burst (SGRB) hosts included in the galaxy sample show N/H<=0.04 solar and O/H solar. They seem to continue the low bound N/H trend of SN hosts at z<0.3. The distribution of N/O as a function of metallicity for SN and LGRB hosts is compared with star chemical evolution models. The results show that several LGRB hosts can be explained by star multibursting models when 12+log(O/H)<8.5, while some objects follow the trend of continuous star formation models. N/O in SN hosts at log(O/H)+12<8.5 are not well explained by stellar chemical evolution models calculated for starburst galaxies. At 12+log(O/H)>8.5 many different objects are nested close to O/H solar with N/O ranging between the maximum corresponding to starburst galaxies and AGN and the minimum corresponding to HII regions and SGRB.2017MNRAS.469.3125Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/469/3125CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/469/3125https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/469/3125http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/469/3125https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/469/3125https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/469/3125http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/469/3125GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/469/3125/table1 (Modelling line ratios to H{beta}=1 from the CALIFA HII regions (Marino et al., 2013, Cat. J/A+A/559/A114))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/469/3125/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/469/3125/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/469/3125/table1?GETtext/xml+votable180.050000true321.499175-3.80986110.005555555555555556Cone search capability for table J/MNRAS/469/3125/table3 (Modelling line ratios to H{beta}=1 from the HII regions of Berg et al. (2012ApJ...754...98B))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/469/3125/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/469/3125/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/469/3125/table3?GETtext/xml+votable180.050000true21.14070831.73146390.005555555555555556Cone search capability for table J/MNRAS/469/3125/table5 (Modelling line ratios to H{beta}=1 of AGN spectra at z<=0.1 (Dors et al. 2017MNRAS.468L.113D))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/469/3125/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/469/3125/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/469/3125/table5?GETtext/xml+votable180.050000true220.158741753.50451110.005555555555555556Cone search capability for table J/MNRAS/469/3125/table7 (Modelling line ratios to H{beta}=1 of Type I SN host spectra at z<=0.03 (Gallagher et al., 2005ApJ...634..210G))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/469/3125/table7?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/469/3125/table7?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/469/3125/table7?GETtext/xml+votable180.050000true188.62320832.19980560.0055555555555555566/34 396 2130 2229 4181 4439 5584 5639 5970 5975 5978 6604-6605 6609 6623 6936 7091 7446 7607 7649 7741 7869 7921 7956 8064 9144 9614 10215 10221 10265 10336 10348 10674 10734 10755 10793 10858 10910-10911 10959 10984 10999 11092 11120 11416 11434 11444 11544 11886 11933 11989 12199 13120 13637 13707 17529 17614 17850 17991 18032 18081 18184 18206 18296 18365 18398 18419 18934 19073 19130 19538 19551 19581 20193 24750 25078 26271 26336 27055 27375 27465 27918 28167 28299 28498 28610 28617 28636 28666 30027 31628 32129 35284 35691 35717 36618 38668 42016 42120 44001 44007 44026 45735 46442https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/469/3125?format=asciiGamma-raydefaultJ/MNRAS/469/3125/table1Modelling line ratios to H{beta}=1 from the CALIFA HII regions (Marino et al., 2013, Cat. J/A+A/559/A114)SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameHII region or model namemeta.id;meta.maincharz? Redshiftsrc.redshiftdoublenullable[OII]3727+Line ratio [OII]3727/H{beta}spect.line.intensity;arith.ratiofloat[OIII]4363Line ratio [OII]4363/H{beta}spect.line.intensity;arith.ratiofloat[OIII]5007Line ratio [OII]5007/H{beta}spect.line.intensity;arith.ratiofloat[NII]6583Line ratio [NII]6583/H{beta}spect.line.intensity;arith.ratiofloatFHb? H{beta} flux (in 10^-16^erg/cm^2^/s)1e-19W.m**-2phot.flux;em.line.Hbetafloatnullable_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullableJ/MNRAS/469/3125/table2Models used to reproduce the spectra presented in Table 1ModelModel namemeta.id;stat.param;meta.modelledcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintn_Model[2] 2: calculated by inflowmeta.notecharVsShock velocitykm/sphys.velocintn0Atomic pre-shock densitycm**-3phys.densityintDGeometrical thickness1e+18cmsrc.morph.paramfloatN/HN/H relative abundancephys.abundfloatO/HO/H relative abundancephys.abundfloatT*Effective temperature10000Kphys.temperature.effectivefloatUIonisation parameterstat.paramfloatFHbH{beta} flux, calculated at the nebula (in erg/cm^2^/s)mW.m**-2phot.flux;em.line.HbetafloatJ/MNRAS/469/3125/table3Modelling line ratios to H{beta}=1 from the HII regions of Berg et al. (2012ApJ...754...98B)SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameHII region or model namemeta.id;meta.maincharz? Redshiftsrc.redshiftdoublenullable[OII]3727+Line ratio[OII]3727/H{beta}spect.line.intensity;arith.ratiofloat[NeIII]3869+? Line ratio [NeIII]3869/H{beta}spect.line.intensity;arith.ratiofloatnullableHgLine ratio H{gamma}(4340)/H{beta}spect.line.intensity;arith.ratiofloat[OIII]4363? Line ratio [OIII]4363/H{beta}spect.line.intensity;arith.ratiofloatnullable[OIII]5007+Line ratio [OIII]5007/H{beta}spect.line.intensity;arith.ratiofloatHeI? Line ratio HeI5876/H{beta}spect.line.intensity;arith.ratiofloatnullable[SIII]6312? Line ratio [SIII]6312/H{beta}spect.line.intensity;arith.ratiofloatnullable[OI]6300+? Line ratio [OI]6300/H{beta}spect.line.intensity;arith.ratiofloatnullable[NII]6548+? Line ratio [NII]6548/H{beta}spect.line.intensity;arith.ratiofloatnullableHaLine ratio H{alpha}(6563)/H{beta}spect.line.intensity;arith.ratiofloat[SII]6717? Line ratio [SII]6717/H{beta}spect.line.intensity;arith.ratiofloatnullable[SII]6731? Line ratio [SII]6731/H{beta}spect.line.intensity;arith.ratiofloatnullable_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullableJ/MNRAS/469/3125/table4Models used to reproduce the spectra presented in Table 3VsShock velocitykm/sphys.velocintUIonisation parameterstat.paramfloatModelModel namemeta.id;stat.param;meta.modelledcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintn0Atomic pre-shock densitycm**-3phys.densityintDGeometrical thickness1e+18cmsrc.morph.paramfloatN/HN/H relative abundancephys.abundfloatO/HO/H relative abundancephys.abundfloatNe/HNe/H relative abundancephys.abundfloatS/HS/H relative abundancephys.abundfloatT*Effective temperature1000Kphys.temperature.effectivefloatFHbH{beta} flux, calculated at the nebula (in erg/cm^2^/s)mW.m**-2phot.flux;em.line.HbetafloatJ/MNRAS/469/3125/table5Modelling line ratios to H{beta}=1 of AGN spectra at z<=0.1 (Dors et al. 2017MNRAS.468L.113D)SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAGN or model namemeta.id;meta.maincharz? Redshiftsrc.redshiftdoublenullable[OII]3727+Line ratio [OII]3727/H{beta}spect.line.intensity;arith.ratiofloat[OIII]5007+Line ratio [OIII]5007/H{beta}spect.line.intensity;arith.ratiofloat[NII]6583+Line ratio [NII]6583/H{beta}spect.line.intensity;arith.ratiofloat[SII]6719+Line ratio [SII]6719/H{beta}spect.line.intensity;arith.ratiofloatRef[1/4]? References (1)meta.refintnullable_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullableJ/MNRAS/469/3125/table6Models used to reproduce the spectra presented in Table 5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintModelModel namemeta.id;stat.param;meta.modelledcharVsShock velocitykm/sphys.velocintn0Atomic pre-shock densitycm**-3phys.densityintFFlux at the Lyman limit1e+10ph.cm**-2.s**-1.eV**-1phot.flux;em.UVfloatDGeometrical thickness1e+17cmsrc.morph.paramfloatN/HN/H relative abundancephys.abundfloatO/HO/H relative abundancephys.abundfloatS/HS/H relative abundancephys.abundfloatFHbB{beta} flux, calculated at the nebula (in erg/cm^2^/s)mW.m**-2phot.flux;em.line.HbetafloatJ/MNRAS/469/3125/table7Modelling line ratios to H{beta}=1 of Type I SN host spectra at z<=0.03 (Gallagher et al., 2005ApJ...634..210G)SimbadNameSimbad column added by the CDSmeta.idcharz? Redshiftsrc.redshiftfloatnullableNameHost galaxy or model namemeta.id.parentcharSNSupernova namemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[OII]3727+Line ratio [OII]3727/H{beta}spect.line.intensity;arith.ratiofloat[OIII]5007+Line ratio [OII]5007/H{beta}spect.line.intensity;arith.ratiofloat[OI]6300Line ratio [OI]6300/H{beta}spect.line.intensity;arith.ratiofloat[NII]6548+Line ratio [NII]6548/H{beta}spect.line.intensity;arith.ratiofloatHaLine ratio H{alpha}(6563)/H{beta}spect.line.intensity;arith.ratiofloat[SII]6717Line ratio [SII]6717/H{beta}spect.line.intensity;arith.ratiofloat[SII]6731Line ratio [SII]6731/H{beta}spect.line.intensity;arith.ratiofloat_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullableJ/MNRAS/469/3125/table8Models used to reproduce the spectra presented in Table 7recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintModelModel namemeta.id;stat.param;meta.modelledcharVsShock velocitykm/sphys.velocintn0Atomic pre-shock densitycm**-3phys.densityintDGeometrical thickness1e+18cmsrc.morph.paramfloatN/HN/H relative abundancephys.abundfloatO/HO/H relative abundancephys.abundfloatS/HS/H relative abundancephys.abundfloatT*Effective temperature10000Kphys.temperature.effectivefloatUIonisation parameterstat.paramfloatFHbH{beta} flux, calculated at the nebula (in 10^-3^erg/cm^2^/s)1e-06W.m**-2phot.flux;em.line.Hbetafloat