We have been carrying out a systematic survey of the star formation and ISM
properties in the host galaxies of z~6 quasars. Our 250 GHz observations,
together with available data from the literature, yield a sample of 14 z~6
quasars that are bright in millimeter dust continuum emission with estimated
FIR luminosities of a few 10^12 to 10^13 Lsun. Most of these
millimeter-detected z~6 quasars have also been detected in molecular CO line
emission, indicating molecular gas masses on order of 10^10 Msun. We have
searched for C II 158 micron fine structure line emission toward four of the
millimeter bright z~6 quasars with ALMA and all of them have been detected. All
these results suggest massive star formation at rates of about 600 to 2000
Msun/yr over the central few kpc region of these quasar host galaxies.
Description
[1210.0242] Star Formation in Quasar Host Galaxies at Redshift 6: Millimeter Surveys and New Insights from ALMA
%0 Generic
%1 wang2012formation
%A Wang, Ran
%A Wagg, Jeff
%A Carilli, Chris L.
%A Walter, Fabian
%A Fan, Xiaohui
%A Bertoldi, Frank
%A Riechers, Dominik. A.
%A Omont, Alain
%A Menten, Karl M.
%A Cox, Pierre
%A Strauss, Michael A.
%A Narayanan, Desika
%D 2012
%K formation gas high-z molecular qso star
%T Star Formation in Quasar Host Galaxies at Redshift 6: Millimeter Surveys
and New Insights from ALMA
%U http://arxiv.org/abs/1210.0242
%X We have been carrying out a systematic survey of the star formation and ISM
properties in the host galaxies of z~6 quasars. Our 250 GHz observations,
together with available data from the literature, yield a sample of 14 z~6
quasars that are bright in millimeter dust continuum emission with estimated
FIR luminosities of a few 10^12 to 10^13 Lsun. Most of these
millimeter-detected z~6 quasars have also been detected in molecular CO line
emission, indicating molecular gas masses on order of 10^10 Msun. We have
searched for C II 158 micron fine structure line emission toward four of the
millimeter bright z~6 quasars with ALMA and all of them have been detected. All
these results suggest massive star formation at rates of about 600 to 2000
Msun/yr over the central few kpc region of these quasar host galaxies.
@misc{wang2012formation,
abstract = {We have been carrying out a systematic survey of the star formation and ISM
properties in the host galaxies of z~6 quasars. Our 250 GHz observations,
together with available data from the literature, yield a sample of 14 z~6
quasars that are bright in millimeter dust continuum emission with estimated
FIR luminosities of a few 10^12 to 10^13 Lsun. Most of these
millimeter-detected z~6 quasars have also been detected in molecular CO line
emission, indicating molecular gas masses on order of 10^10 Msun. We have
searched for [C II] 158 micron fine structure line emission toward four of the
millimeter bright z~6 quasars with ALMA and all of them have been detected. All
these results suggest massive star formation at rates of about 600 to 2000
Msun/yr over the central few kpc region of these quasar host galaxies.},
added-at = {2012-10-02T19:37:10.000+0200},
author = {Wang, Ran and Wagg, Jeff and Carilli, Chris L. and Walter, Fabian and Fan, Xiaohui and Bertoldi, Frank and Riechers, Dominik. A. and Omont, Alain and Menten, Karl M. and Cox, Pierre and Strauss, Michael A. and Narayanan, Desika},
biburl = {https://www.bibsonomy.org/bibtex/2e8c5ba603474f8a9d7bd1cd13b611911/miki},
description = {[1210.0242] Star Formation in Quasar Host Galaxies at Redshift 6: Millimeter Surveys and New Insights from ALMA},
interhash = {632bdf686dafbab67973c945e024b7f1},
intrahash = {e8c5ba603474f8a9d7bd1cd13b611911},
keywords = {formation gas high-z molecular qso star},
note = {cite arxiv:1210.0242Comment: 4 pages, 2 figures, submitted to Preceedings IAU Symposium No. 292 "Molecular Gas, Dust, and Star Formation in Galaxies"},
timestamp = {2012-10-02T19:37:10.000+0200},
title = {Star Formation in Quasar Host Galaxies at Redshift 6: Millimeter Surveys
and New Insights from ALMA},
url = {http://arxiv.org/abs/1210.0242},
year = 2012
}