CI, [CII] and CO observations towards TNJ 1338–1942: Probing the ISM in a massive proto-cluster galaxy at z = 4.11

S König; T R Greve; N Seymour; J I Rawlings; P Papadopoulos; R J Ivison; C De Breuck; J Stevens; I Smail; A Kovacs

CI, [CII] and CO observations towards TNJ 1338–1942: Probing the ISM in a massive proto-cluster galaxy at z = 4.11

S König, T R Greve, N Seymour, J I Rawlings, P Papadopoulos, R J Ivison, C De Breuck, J Stevens, I Smail, A Kovacs

DARK

Abstract

A number of studies have dealt with the link between distant powerful radio sources and the most massive galaxies in the early Universe. Despite major advances in our understanding of high redshift radio galaxies (HzRGs), we still only have a rudimentary picture of the physical conditions (i.e. gas density, temperature, ambient UV-field) prevailing in the interstellar medium (ISM) of these objects. Here we report on ongoing CI, [CII] and CO observations of TNJ 1338–1942 at z = 4.11 with the IRAM 30m telescope, the JCMT and ATCA. With these observations we will make a first attempt at constraining the average ISM conditions in TNJ 1338–1942.

Originalsprog	Engelsk
Artikelnummer	012064
Bogserie	Journal of Physics: Conference Series (Online)
Vol/bind	372
Udgave nummer	1
Antal sider	6
ISSN	1742-6596
Status	Udgivet - 2012

Adgang til dokumentet

http://stacks.iop.org/1742-6596/372/i=1/a=012064

Citationsformater

König, S., Greve, T. R., Seymour, N., Rawlings, J. I., Papadopoulos, P., Ivison, R. J., Breuck, C. D., Stevens, J., Smail, I., & Kovacs, A. (2012). CI, [CII] and CO observations towards TNJ 1338–1942: Probing the ISM in a massive proto-cluster galaxy at z = 4.11. Journal of Physics: Conference Series (Online), 372(1), [012064]. http://stacks.iop.org/1742-6596/372/i=1/a=012064

König, S, Greve, TR, Seymour, N, Rawlings, JI, Papadopoulos, P, Ivison, RJ, Breuck, CD, Stevens, J, Smail, I & Kovacs, A 2012, 'CI, [CII] and CO observations towards TNJ 1338–1942: Probing the ISM in a massive proto-cluster galaxy at z = 4.11', Journal of Physics: Conference Series (Online), bind 372, nr. 1, 012064. <http://stacks.iop.org/1742-6596/372/i=1/a=012064>

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abstract = "A number of studies have dealt with the link between distant powerful radio sources and the most massive galaxies in the early Universe. Despite major advances in our understanding of high redshift radio galaxies (HzRGs), we still only have a rudimentary picture of the physical conditions (i.e. gas density, temperature, ambient UV-field) prevailing in the interstellar medium (ISM) of these objects. Here we report on ongoing CI, [CII] and CO observations of TNJ 1338–1942 at z = 4.11 with the IRAM 30m telescope, the JCMT and ATCA. With these observations we will make a first attempt at constraining the average ISM conditions in TNJ 1338–1942.",

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T1 - CI, [CII] and CO observations towards TNJ 1338–1942: Probing the ISM in a massive proto-cluster galaxy at z = 4.11

AU - König, S

AU - Greve, T R

AU - Seymour, N

AU - Rawlings, J I

AU - Papadopoulos, P

AU - Ivison, R J

AU - Breuck, C De

AU - Stevens, J

AU - Smail, I

AU - Kovacs, A

PY - 2012

Y1 - 2012

N2 - A number of studies have dealt with the link between distant powerful radio sources and the most massive galaxies in the early Universe. Despite major advances in our understanding of high redshift radio galaxies (HzRGs), we still only have a rudimentary picture of the physical conditions (i.e. gas density, temperature, ambient UV-field) prevailing in the interstellar medium (ISM) of these objects. Here we report on ongoing CI, [CII] and CO observations of TNJ 1338–1942 at z = 4.11 with the IRAM 30m telescope, the JCMT and ATCA. With these observations we will make a first attempt at constraining the average ISM conditions in TNJ 1338–1942.

AB - A number of studies have dealt with the link between distant powerful radio sources and the most massive galaxies in the early Universe. Despite major advances in our understanding of high redshift radio galaxies (HzRGs), we still only have a rudimentary picture of the physical conditions (i.e. gas density, temperature, ambient UV-field) prevailing in the interstellar medium (ISM) of these objects. Here we report on ongoing CI, [CII] and CO observations of TNJ 1338–1942 at z = 4.11 with the IRAM 30m telescope, the JCMT and ATCA. With these observations we will make a first attempt at constraining the average ISM conditions in TNJ 1338–1942.

M3 - Conference article

SN - 1742-6588

VL - 372

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

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M1 - 012064

ER -