J/ApJ/725/2270     Mid-IR emission lines in AGNs      (Pereira-Santaella+, 2010)

The mid-infrared high-ionization lines from active galactic nuclei and star-forming galaxies. Pereira-Santaella M., Diamond-Stanic A.M., Alonso-Herrero A., Rieke G.H. <Astrophys. J., 725, 2270-2280 (2010)> =2010ApJ...725.2270P 2010ApJ...725.2270P
ADC_Keywords: Active gal. nuclei ; Galaxies, IR ; Galaxies, spectra ; Spectra, infrared Keywords: galaxies: active - galaxies: nuclei - galaxies: starburst - infrared: galaxies Abstract: We used Spitzer/Infrared Spectrograph spectroscopic data on 426 galaxies including quasars, Seyferts, LINERs, and HII galaxies to investigate the relationship among the mid-IR emission lines. There is a tight linear correlation between the [NeV]14.3um and 24.3um (97.1eV) and the [OIV]25.9um (54.9eV) high-ionization emission lines. The correlation also holds for these high-ionization emission lines and the [NeIII]15.56um (41eV) emission line, although only for active galaxies. We used these correlations to calculate the [NeIII] excess due to star formation in Seyfert galaxies. We also estimated the [OIV] luminosity due to star formation in active galaxies and determined that it dominates the [OIV] emission only if the contribution of the active nucleus to the total luminosity is below 5%. We find that the active galactic nucleus dominates the [OIV] emission in most Seyfert galaxies, whereas star formation adequately explains the observed [OIV] emission in optically classified HII galaxies. Finally, we computed photoionization models to determine the physical conditions of the narrow-line region where these high-ionization lines originate. The estimated ionization parameter range is -2.8<logU←2.5 and the total hydrogen column density range is 20<lognH(cm-2)<21. Description: The sample contains 426 galaxies for which high spectral resolution (R∼600) Spitzer/IRS spectra were available, either in the literature, in the Spitzer archive, or observed through the programs 40936 and 50597 (PI: G. H. Rieke). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 106 426 Sample and mid-infrared emission line fluxes -------------------------------------------------------------------------------- See also: VII/157 : The Extended 12um galaxy sample (Rush+ 1993) J/MNRAS/414/500 : Spitzer/IRS ATLAS project source (Hernan-Caballero+, 2011) J/ApJ/719/1191 : Mid-IR indicators of SF and AGN in galaxies (Treyer+, 2010) J/ApJ/723/895 : IR luminosities and aromatic features of 5MUSES (Wu+, 2010) J/ApJ/709/1257 : Spitzer-IRS spectra of Seyfert galaxies (Tommasin+, 2010) J/ApJ/693/1821 : The Spitzer infrared nearby galaxies survey (Dale+, 2009) J/ApJS/182/628 : Spitzer quasar and ULIRG evolution study (Veilleux+, 2009) J/MNRAS/398/1165 : AGN in nearby galaxies (Goulding+, 2009) J/ApJS/184/230 : Spitzer high-resolution MIR spectral atlas (Bernard-Salas+, 2009) J/ApJ/701/1123 : MIR spectroscopic catalog of 150 galaxies (Dasyra+, 2009) J/ApJ/705/14 : Seyfert galaxies in the mid-IR (Deo+, 2009) J/ApJ/658/778 : Spitzer mid-IR spectroscopy of z∼2 ULIRGs (Yan+, 2007) J/ApJS/112/315 : Spectroscopic parameters of Seyfert nuclei (Ho+ 1997) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 --- Name Object name 21- 22 A2 --- f_Name [cd ] Member of other samples (1) 24- 25 I2 h RAh NED Hour of Right Ascension (J2000) 27- 28 I2 min RAm NED Minute of Right Ascension (J2000) 30- 33 F4.1 s RAs NED Second of Right Ascension (J2000) 35 A1 --- DE- Sign of the NED Declination (J2000) 36- 37 I2 deg DEd NED Degree of Declination (J2000) 39- 40 I2 arcmin DEm NED Arcminute of Declination (J2000) 42- 43 I2 arcsec DEs NED Arcsecond of Declination (J2000) 45- 51 F7.2 Mpc Dist Distance (2) 53- 57 A5 --- Class NED spectral classification (H2, LINER, QSO, Sy1 or Sy2) 59- 66 F8.3 10-17W/m2 NeII ? The [NeII] 12.81 micron line flux (3) 68 A1 --- l_NeV-14 Limit flag on NeV-14 69- 76 F8.4 10-17W/m2 NeV-14 The [NeV] 14.32 micron line flux (3) 78- 85 F8.3 10-17W/m2 NeIII ? The [NeIII] 15.56 micron line flux (3) 87 A1 --- l_NeV-24 Limit flag on NeV-24 88- 94 F7.3 10-17W/m2 NeV-24 ? The [NeV] 24.32 micron line flux (3) 96 A1 --- l_OIV Limit flag OIV 97-104 F8.3 10-17W/m2 OIV ? The [OIV] 25.89 micron line flux (3) 106 I1 --- Ref Reference (4) -------------------------------------------------------------------------------- Note (1): Flag as follows: c = Member of the RSA sample (relatively low-luminosity Seyferts; Maiolino & Rieke 1995ApJ...454...95M 1995ApJ...454...95M; Ho et al. 1997, Cat. J/ApJS/112/315; Diamond-Stanic et al. 2009ApJ...698..623D 2009ApJ...698..623D). d = Member of the 12 micron sample (typical Seyfert galaxies; Rush et al. 1993, Cat. VII/157; Tommasin et al. 2010, Cat. J/ApJ/709/1257). Note (2): We calculated the distance from the redshift assuming a flat cosmology with H0=70km/s/Mpc, ΩM=0.3, and ΩΛ=0.7. Except for the galaxies from Dale et al. (2009, Cat. J/ApJ/693/1821), Bernard-Salas et al. (2009, Cat. J/ApJS/184/230) and Goulding & Alexander (2009, Cat. J/MNRAS/398/1165) for which we used the distances adopted by these authors. Note (3): In units of 10-14erg/s/cm2. Note (4): Reference as follows: 1 = Veilleux et al. (2009, Cat. J/ApJS/182/628; QUEST sample); 2 = This work; 3 = Farrah et al. (2007ApJ...667..149F 2007ApJ...667..149F) 4 = Tommasin et al. (2008ApJ...676..836T 2008ApJ...676..836T, 2010, Cat. J/ApJ/709/1257); 5 = Dale et al. (2009, Cat. J/ApJ/693/1821) 6 = Gorjian et al. (2007ApJ...655L..73G 2007ApJ...655L..73G); 7 = Goulding & Alexander (2009, Cat. J/MNRAS/398/1165); 8 = Bernard-Salas et al. (2009, Cat. J/ApJS/184/230). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 10-Aug-2012
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