BAL phosphorus abundance and evidence for immense ionic column densities in quasar outflows: vlt/x-shooter observations of quasar SDSS J1512+1119
dc.contributor | Virginia Tech | en |
dc.contributor.author | Borguet, Benoit C. J. | en |
dc.contributor.author | Edmonds, Douglas | en |
dc.contributor.author | Arav, Nahum | en |
dc.contributor.author | Benn, C. | en |
dc.contributor.author | Chamberlain, Carter | en |
dc.contributor.department | Physics | en |
dc.date.accessed | 2014-02-05 | en |
dc.date.accessioned | 2014-02-25T13:57:02Z | en |
dc.date.available | 2014-02-25T13:57:02Z | en |
dc.date.issued | 2012-10 | en |
dc.description.abstract | We present spectroscopic analysis of the broad absorption line (BAL) outflow in quasar SDSS J1512+1119. In particular, we focus our attention on a kinematic component in which we identify P V and S IV/S IV* absorption troughs. The shape of the unblended phosphorus doublet troughs and the three S IV/S IV* troughs allow us to obtain reliable column density measurements for these two ions. Photoionization modeling using these column densities and those of He I* constrain the abundance of phosphorus to the range of 0.5-4 times the solar value. The total column density, ionization parameter, and metallicity inferred from the P V and S IV column densities lead to large optical depth values for the common transition observed in BAL outflows. We show that the true C IV optical depth is similar to 1000 times greater in the core of the absorption profile than the value deduced from its apparent optical depth. | en |
dc.description.sponsorship | NASA STScI GO 11686, GO 12022 | en |
dc.description.sponsorship | NSF AST 0837880 | en |
dc.identifier.citation | Benoit C. J. Borguet et al. 2012. "BAL phosphorus abundance and evidence for immense ionic column densities in quasar outflows: vlt/x-shooter observations of quasar SDSS J1512+1119," ApJ 758 69 doi:10.1088/0004-637X/758/1/69 | en |
dc.identifier.doi | https://doi.org/10.1088/0004-637x/758/1/69 | en |
dc.identifier.issn | 0004-637X | en |
dc.identifier.uri | http://hdl.handle.net/10919/25534 | en |
dc.identifier.url | http://m.iopscience.iop.org/0004-637X/758/1/69/pdf/0004-637X_758_1_69.pdf | en |
dc.language.iso | en_US | en |
dc.publisher | IOP Publishing Ltd. | en |
dc.rights | In Copyright | en |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | en |
dc.subject | galaxies: individual (sdss j1512+1119) | en |
dc.subject | line: formation | en |
dc.subject | quasars: | en |
dc.subject | absorption lines | en |
dc.subject | space-telescope observations | en |
dc.subject | galactic nucleus outflows | en |
dc.subject | absorption-line | en |
dc.subject | quasars | en |
dc.subject | keck hires observations | en |
dc.subject | c-iv absorption | en |
dc.subject | intrinsic absorption | en |
dc.subject | metal abundances | en |
dc.subject | ultraviolet-absorption | en |
dc.subject | chemical abundances | en |
dc.subject | stis | en |
dc.subject | observations | en |
dc.title | BAL phosphorus abundance and evidence for immense ionic column densities in quasar outflows: vlt/x-shooter observations of quasar SDSS J1512+1119 | en |
dc.title.serial | Astrophysical Journal | en |
dc.type | Article - Refereed | en |
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