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Outflow in Overlooked Luminous Quasar: Subaru Observations of AKARI J1757+5907
by
Matsuhara, Hideo
, Aoki, Kentaro
, Arav, Nahum
, Korista, Kirk T
, Toba, Yoshiki
, Dunn, Jay P
, Oyabu, Shinki
, Edmonds, Doug
in
Absorption
/ Density
/ Ionization
/ Luminosity
/ Mass flow rate
/ Outflow
/ Photoionization
/ Quasars
/ Starburst galaxies
2011
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Outflow in Overlooked Luminous Quasar: Subaru Observations of AKARI J1757+5907
by
Matsuhara, Hideo
, Aoki, Kentaro
, Arav, Nahum
, Korista, Kirk T
, Toba, Yoshiki
, Dunn, Jay P
, Oyabu, Shinki
, Edmonds, Doug
in
Absorption
/ Density
/ Ionization
/ Luminosity
/ Mass flow rate
/ Outflow
/ Photoionization
/ Quasars
/ Starburst galaxies
2011
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While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
Outflow in Overlooked Luminous Quasar: Subaru Observations of AKARI J1757+5907
by
Matsuhara, Hideo
, Aoki, Kentaro
, Arav, Nahum
, Korista, Kirk T
, Toba, Yoshiki
, Dunn, Jay P
, Oyabu, Shinki
, Edmonds, Doug
in
Absorption
/ Density
/ Ionization
/ Luminosity
/ Mass flow rate
/ Outflow
/ Photoionization
/ Quasars
/ Starburst galaxies
2011
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Outflow in Overlooked Luminous Quasar: Subaru Observations of AKARI J1757+5907
Paper
Outflow in Overlooked Luminous Quasar: Subaru Observations of AKARI J1757+5907
2011
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Overview
We present Subaru observations of the newly discovered luminous quasar AKARI J1757+5907, which shows an absorption outflow in its spectrum. The absorption consists of 9 distinct troughs, and our analysis focuses on the troughs at ~ -1000$ km s^-1 for which we can measure accurate column densities of He I*, Fe II and Mg II. We use photoionization models to constrain the ionization parameter, total hydrogen column density, and the number density of the outflowing gas. These constraints yield lower limits for the distance, mass flow rate and kinetic luminosity for the outflow of 3.7 kpc, 70 M_sun yr^-1, and 2.0 x 10^43 ergs s^-1, respectively. Such mass flow rate value can contribute significantly to the metal enrichment of the intra-cluster medium. We find that this moderate velocity outflow is similar to those recently discovered in massive post-starburst galaxies. Finally, we describe the scientific potential of future observations targeting this object.
Publisher
Cornell University Library, arXiv.org
Subject
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