A1 Refereed original research article in a scientific journal
On the cool gaseous haloes of quasars
Authors: Farina EP, Falomo R, Decarli R, Treves A, Kotilainen JK
Publisher: OXFORD UNIV PRESS
Publication year: 2013
Journal: Monthly Notices of the Royal Astronomical Society
Journal name in source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Journal acronym: MON NOT R ASTRON SOC
Number in series: 2
Volume: 429
Issue: 2
First page : 1267
Last page: 1277
Number of pages: 11
ISSN: 0035-8711
DOI: https://doi.org/10.1093/mnras/sts410
Abstract
We present the optical spectroscopy of projected quasar (QSO) pairs in order to investigate the MgII and CIV absorption features imprinted on the spectrum of the background object by the gaseous halo surrounding the foreground QSO. We have observed 13 projected pairs in the redshift range 0.7 <= zF <= 2.2, spanning projected separations between 60 and 120 kpc. In the spectra of the background QSOs, we have identified MgII intervening absorption systems associated with the foreground QSOs in seven out of 10 pairs, and one absorption system out of three is found for C IV. The distribution of the equivalent width (EW) as a function of the impact parameter shows that, unlike the case of normal galaxies, some strong absorption systems (EWr > 1 angstrom) are also present beyond a projected radius of similar to 70 kpc. If we take into account the mass of the galaxies as an additional parameter that influences the extent of the gaseous haloes, the distribution of the absorptions connected to the QSOs is consistent with that of galaxies. In the spectra of the foreground QSOs, we do not detect any Mg II absorption lines originated by the gas surrounding the QSO itself, but in two cases, these features are present for CIV. A comparison between the absorption features observed in the transverse direction and those along the line of sight allows us to comment on the distribution of the absorbing gas and on the emission properties of the QSOs.
We present the optical spectroscopy of projected quasar (QSO) pairs in order to investigate the MgII and CIV absorption features imprinted on the spectrum of the background object by the gaseous halo surrounding the foreground QSO. We have observed 13 projected pairs in the redshift range 0.7 <= zF <= 2.2, spanning projected separations between 60 and 120 kpc. In the spectra of the background QSOs, we have identified MgII intervening absorption systems associated with the foreground QSOs in seven out of 10 pairs, and one absorption system out of three is found for C IV. The distribution of the equivalent width (EW) as a function of the impact parameter shows that, unlike the case of normal galaxies, some strong absorption systems (EWr > 1 angstrom) are also present beyond a projected radius of similar to 70 kpc. If we take into account the mass of the galaxies as an additional parameter that influences the extent of the gaseous haloes, the distribution of the absorptions connected to the QSOs is consistent with that of galaxies. In the spectra of the foreground QSOs, we do not detect any Mg II absorption lines originated by the gas surrounding the QSO itself, but in two cases, these features are present for CIV. A comparison between the absorption features observed in the transverse direction and those along the line of sight allows us to comment on the distribution of the absorbing gas and on the emission properties of the QSOs.
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