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J/ApJ/709/611       The multi-component absorber QSO 0318-0600     (Dunn+, 2010)

The quasar outflow contribution to AGN feedback: VLT measurements of SDSS J0318-0600. Dunn J.P., Bautista M., Arav N., Moe M., Korista K., Costantini E., Benn C., Ellison S., Edmonds D. <Astrophys. J., 709, 611-631 (2010)> =2010ApJ...709..611D
ADC_Keywords: QSOs ; Spectroscopy ; Line Profiles Keywords: quasars: absorption lines - quasars: individual (SDSS J0318-0600) Abstract: We present high spectral resolution Very Large Telescope observations of the broad absorption line quasar SDSS J0318-0600. This high-quality data set allows us to extract accurate ionic column densities and determine an electron number density of ne=103.3±0.2cm-3 for the main outflow absorption component. The heavily reddened spectrum of SDSS J0318-0600 requires purely silicate dust with a reddening curve characteristic of predominately large grains, from which we estimate the bolometric luminosity. We carry out photoionization modeling to determine the total column density, ionization parameter, and distance of the gas and find that the photoionization models suggest abundances greater than solar. Due to the uncertainty in the location of the dust extinction, we arrive at two viable distances for the main ouflow component from the central source, 6 and 17kpc, where we consider the 6kpc location as somewhat more physically plausible. Assuming the canonical global covering of 20% for the outflow and a distance of 6kpc, our analysis yields a mass flux of 120M/yr and a kinetic luminosity that is ∼0.1% of the bolometric luminosity of the object. Should the dust be part of the outflow, then these values are ∼4x larger. The large mass flux and kinetic luminosity make this outflow a significant contributor to active galactic nucleus feedback processes. Description: During 2006 October (September 30 to October 22), we obtained eight echelle spectra, each with an exposure time of 2850s, of the object SDSS J0318-0600 (z=1.967, Schneider et al. 2007, Cat. VII/260, RA=031856.7, DE=-060037.4) with the VLT. The spectra were taken using the UV-Visual Echelle Spectrograph (UVES) with a slit width of 1.0" which gives a resolving power of ∼40000, and a central wavelength position of 5800 and 3460Å for the red and blue detectors respectively. Objects: -------------------------------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------------------------------- 03 18 56.63 -06 00 37.7 QSO 0318-0600 = SDSS J031856.62-060037.7 -------------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 43 91 Detected absorption lines in QSO 0318-0600
See also: VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010) J/MNRAS/410/860 : Redshift dependence of BAL QSOs (Allen+, 2011) J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010) J/A+A/508/1527 : SiII Radiative transition rates (Bautista+, 2009) J/MNRAS/382/412 : Catalog of SDSS-DR5/2MASS spectroscopic quasars (Ofek, 2007) J/PASP/118/1077 : Metal-strong damped Lyα systems (Herbert-Fort+, 2006) http://www.nist.gov/pml/data/asd.cfm : NIST Atomic Spectra Database Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 6 A6 --- Ion Ion identification 8- 14 F7.2 0.1nm lambda Wavelength in Angstroms 16- 21 F6.3 [-] log(gf) Log of the oscillator strength 23- 27 I5 cm-1 Elow Energy of lower level 29- 30 I2 --- glow Lower level 32- 40 A9 --- Comp Kinematic components measured (labeled a-k from high to low velocity) 42- 43 I2 --- Ref Reference (1)
Note (1): Reference as follows: 1 = Bautista et al. (2009MNRAS.393.1503B); 2 = Bautista et al. (2009, to be submitted); 3 = Kurucz & Bell (1995all..book.....K); 4 = K. Butler, C. Mendoza, and C. J. Zeippen, J. Phys. B 26, 4409 (1993); 5 = C. E. Moore, NSRDS-NBS 3, Sect. 3 (1970ipil.book.....M); 6 = Fedchak & Lawler (1999ApJ...523..734F); 7 = Fedchak, Wiese, Lawler (2000ApJ...538..773F ); 8 = J. R. Fuhr and W. L. Wiese, Atomic Transition Probabilities, published in the CRC Handbook of Chemistry and Physics, 79th Edition, edited by D. R. Lide (CRC Press, Inc., Boca Raton, FL, 1998); 9 = Fuhr & Wiese (2006, J. Chem. Ref. Data, Vol. 35, No.4)) 10 = NIST Atomic Spectra Database (2009 - http://www.nist.gov/pml/data/asd.cfm); 11 = Salih, Lawler, Whaling 1985, Phys Rev A 31, 744; 12 = Toner & Hibbert (2005MNRAS.361..673T).
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 05-Mar-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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