A Mini-BAL Outflow at 900 pc from the Central Source: VLT/X-shooter Observations

We determine the physical conditions and location of the outflow material seen in the mini-BAL quasar SDSS J1111+1437 (z = 2.138). These results are based on the analysis of a high S/N, medium-resolution VLT/X-shooter spectrum. The main outflow component spans the velocity range −1500 to −3000 km s−...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal 2018-05, Vol.858 (1), p.39
Hauptverfasser: Xu, Xinfeng, Arav, Nahum, Miller, Timothy, Benn, Chris
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 1
container_start_page 39
container_title The Astrophysical journal
container_volume 858
creator Xu, Xinfeng
Arav, Nahum
Miller, Timothy
Benn, Chris
description We determine the physical conditions and location of the outflow material seen in the mini-BAL quasar SDSS J1111+1437 (z = 2.138). These results are based on the analysis of a high S/N, medium-resolution VLT/X-shooter spectrum. The main outflow component spans the velocity range −1500 to −3000 km s−1 and has detected absorption troughs from both high-ionization species: C iv, N v, O vi, Si iv, P v, and S iv; and low-ionization species: H i, C ii, Mg ii, Al ii, Al iii, Si ii, and Si iii. Measurements of these troughs allow us to derive an accurate photoionization solution for this absorption component: a hydrogen column density, cm−2 and ionization parameter, . Troughs produced from the ground and excited states of S iv combined with the derived value allow us to determine an electron number density of cm−3 and to obtain the distance of the ionized gas from the central source: pc.
doi_str_mv 10.3847/1538-4357/aab7ea
format Article
fullrecord <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_journals_2365933668</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2365933668</sourcerecordid><originalsourceid>FETCH-LOGICAL-c416t-f739c9595879414e28f0e40bdb401b75280bd74c43e2d0f4ba791e2c87206eb3</originalsourceid><addsrcrecordid>eNp1kM1LwzAYxoMoOKd3jwGvxqVJ2jTe5pgfUJngkN1CkiWsY2tqkin-97ZU9OTp_eB5nvflB8Blhm9oyfgky2mJGM35RCnNrToCo9_VMRhhjBkqKF-dgrMYt_1IhBiBlyl8rpsa3U0ruDgkt_OfUCUoMIatgS74PUwbC2e2SUHt4Ks_BGNv4Vu1nKxQ3HifbIALHW34UKn2TTwHJ07tor34qWOwvJ8vZ4-oWjw8zaYVMiwrEnKcCiNykZdcsIxZUjpsGdZrzXCmeU7KrufMMGrJGjumFReZJabkBBdW0zG4GmLb4N8PNia57V5ruouS0CIXlBZF2anwoDLBxxisk22o9yp8yQzLHpvsGcmekRywdZbrwVL79i_zX_k3JS5scg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2365933668</pqid></control><display><type>article</type><title>A Mini-BAL Outflow at 900 pc from the Central Source: VLT/X-shooter Observations</title><source>Institute of Physics Open Access Journal Titles</source><creator>Xu, Xinfeng ; Arav, Nahum ; Miller, Timothy ; Benn, Chris</creator><creatorcontrib>Xu, Xinfeng ; Arav, Nahum ; Miller, Timothy ; Benn, Chris</creatorcontrib><description>We determine the physical conditions and location of the outflow material seen in the mini-BAL quasar SDSS J1111+1437 (z = 2.138). These results are based on the analysis of a high S/N, medium-resolution VLT/X-shooter spectrum. The main outflow component spans the velocity range −1500 to −3000 km s−1 and has detected absorption troughs from both high-ionization species: C iv, N v, O vi, Si iv, P v, and S iv; and low-ionization species: H i, C ii, Mg ii, Al ii, Al iii, Si ii, and Si iii. Measurements of these troughs allow us to derive an accurate photoionization solution for this absorption component: a hydrogen column density, cm−2 and ionization parameter, . Troughs produced from the ground and excited states of S iv combined with the derived value allow us to determine an electron number density of cm−3 and to obtain the distance of the ionized gas from the central source: pc.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/aab7ea</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Absorption ; Aluminum ; Astrophysics ; Density ; galaxies: active ; galaxies: kinematics and dynamics ; Hydrogen ; Ionization ; ISM: jets and outflows ; Magnesium ; Outflow ; Photoionization ; Quasars ; quasars: absorption lines ; Silicon ; Troughs</subject><ispartof>The Astrophysical journal, 2018-05, Vol.858 (1), p.39</ispartof><rights>2018. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing May 01, 2018</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c416t-f739c9595879414e28f0e40bdb401b75280bd74c43e2d0f4ba791e2c87206eb3</citedby><cites>FETCH-LOGICAL-c416t-f739c9595879414e28f0e40bdb401b75280bd74c43e2d0f4ba791e2c87206eb3</cites><orcidid>0000-0002-9217-7051</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/aab7ea/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,780,784,27924,27925,38890,53867</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/aab7ea$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc></links><search><creatorcontrib>Xu, Xinfeng</creatorcontrib><creatorcontrib>Arav, Nahum</creatorcontrib><creatorcontrib>Miller, Timothy</creatorcontrib><creatorcontrib>Benn, Chris</creatorcontrib><title>A Mini-BAL Outflow at 900 pc from the Central Source: VLT/X-shooter Observations</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>We determine the physical conditions and location of the outflow material seen in the mini-BAL quasar SDSS J1111+1437 (z = 2.138). These results are based on the analysis of a high S/N, medium-resolution VLT/X-shooter spectrum. The main outflow component spans the velocity range −1500 to −3000 km s−1 and has detected absorption troughs from both high-ionization species: C iv, N v, O vi, Si iv, P v, and S iv; and low-ionization species: H i, C ii, Mg ii, Al ii, Al iii, Si ii, and Si iii. Measurements of these troughs allow us to derive an accurate photoionization solution for this absorption component: a hydrogen column density, cm−2 and ionization parameter, . Troughs produced from the ground and excited states of S iv combined with the derived value allow us to determine an electron number density of cm−3 and to obtain the distance of the ionized gas from the central source: pc.</description><subject>Absorption</subject><subject>Aluminum</subject><subject>Astrophysics</subject><subject>Density</subject><subject>galaxies: active</subject><subject>galaxies: kinematics and dynamics</subject><subject>Hydrogen</subject><subject>Ionization</subject><subject>ISM: jets and outflows</subject><subject>Magnesium</subject><subject>Outflow</subject><subject>Photoionization</subject><subject>Quasars</subject><subject>quasars: absorption lines</subject><subject>Silicon</subject><subject>Troughs</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNp1kM1LwzAYxoMoOKd3jwGvxqVJ2jTe5pgfUJngkN1CkiWsY2tqkin-97ZU9OTp_eB5nvflB8Blhm9oyfgky2mJGM35RCnNrToCo9_VMRhhjBkqKF-dgrMYt_1IhBiBlyl8rpsa3U0ruDgkt_OfUCUoMIatgS74PUwbC2e2SUHt4Ks_BGNv4Vu1nKxQ3HifbIALHW34UKn2TTwHJ07tor34qWOwvJ8vZ4-oWjw8zaYVMiwrEnKcCiNykZdcsIxZUjpsGdZrzXCmeU7KrufMMGrJGjumFReZJabkBBdW0zG4GmLb4N8PNia57V5ruouS0CIXlBZF2anwoDLBxxisk22o9yp8yQzLHpvsGcmekRywdZbrwVL79i_zX_k3JS5scg</recordid><startdate>20180501</startdate><enddate>20180501</enddate><creator>Xu, Xinfeng</creator><creator>Arav, Nahum</creator><creator>Miller, Timothy</creator><creator>Benn, Chris</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-9217-7051</orcidid></search><sort><creationdate>20180501</creationdate><title>A Mini-BAL Outflow at 900 pc from the Central Source: VLT/X-shooter Observations</title><author>Xu, Xinfeng ; Arav, Nahum ; Miller, Timothy ; Benn, Chris</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c416t-f739c9595879414e28f0e40bdb401b75280bd74c43e2d0f4ba791e2c87206eb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Absorption</topic><topic>Aluminum</topic><topic>Astrophysics</topic><topic>Density</topic><topic>galaxies: active</topic><topic>galaxies: kinematics and dynamics</topic><topic>Hydrogen</topic><topic>Ionization</topic><topic>ISM: jets and outflows</topic><topic>Magnesium</topic><topic>Outflow</topic><topic>Photoionization</topic><topic>Quasars</topic><topic>quasars: absorption lines</topic><topic>Silicon</topic><topic>Troughs</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Xu, Xinfeng</creatorcontrib><creatorcontrib>Arav, Nahum</creatorcontrib><creatorcontrib>Miller, Timothy</creatorcontrib><creatorcontrib>Benn, Chris</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Xu, Xinfeng</au><au>Arav, Nahum</au><au>Miller, Timothy</au><au>Benn, Chris</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Mini-BAL Outflow at 900 pc from the Central Source: VLT/X-shooter Observations</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2018-05-01</date><risdate>2018</risdate><volume>858</volume><issue>1</issue><spage>39</spage><pages>39-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>We determine the physical conditions and location of the outflow material seen in the mini-BAL quasar SDSS J1111+1437 (z = 2.138). These results are based on the analysis of a high S/N, medium-resolution VLT/X-shooter spectrum. The main outflow component spans the velocity range −1500 to −3000 km s−1 and has detected absorption troughs from both high-ionization species: C iv, N v, O vi, Si iv, P v, and S iv; and low-ionization species: H i, C ii, Mg ii, Al ii, Al iii, Si ii, and Si iii. Measurements of these troughs allow us to derive an accurate photoionization solution for this absorption component: a hydrogen column density, cm−2 and ionization parameter, . Troughs produced from the ground and excited states of S iv combined with the derived value allow us to determine an electron number density of cm−3 and to obtain the distance of the ionized gas from the central source: pc.</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/aab7ea</doi><tpages>9</tpages><orcidid>https://orcid.org/0000-0002-9217-7051</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier ISSN: 0004-637X
ispartof The Astrophysical journal, 2018-05, Vol.858 (1), p.39
issn 0004-637X
1538-4357
language eng
recordid cdi_proquest_journals_2365933668
source Institute of Physics Open Access Journal Titles
subjects Absorption
Aluminum
Astrophysics
Density
galaxies: active
galaxies: kinematics and dynamics
Hydrogen
Ionization
ISM: jets and outflows
Magnesium
Outflow
Photoionization
Quasars
quasars: absorption lines
Silicon
Troughs
title A Mini-BAL Outflow at 900 pc from the Central Source: VLT/X-shooter Observations
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-04T04%3A58%3A21IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=A%20Mini-BAL%20Outflow%20at%20900%20pc%20from%20the%20Central%20Source:%20VLT/X-shooter%20Observations&rft.jtitle=The%20Astrophysical%20journal&rft.au=Xu,%20Xinfeng&rft.date=2018-05-01&rft.volume=858&rft.issue=1&rft.spage=39&rft.pages=39-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/1538-4357/aab7ea&rft_dat=%3Cproquest_O3W%3E2365933668%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2365933668&rft_id=info:pmid/&rfr_iscdi=true