ALMA finds dew drops in the dusty spider's web
Artikel i vetenskaplig tidskrift, 2016

We present 0 ''.5 resolution ALMA detections of the observed 246 GHz continuum, [CI] P-3(2) -> P-3(1) fine structure line ([CI] 2-1), CO(7-6), and H2O lines in the z = 2:161 radio galaxy MRC1138-262, the so-called Spiderweb galaxy. We detect strong [CI] 2-1 emission both at the position of the radio core, and in a second component similar to 4 kpc away from it. The 1100 km s(-1) broad [CI]2-1 line in this latter component, combined with its H-2 mass of 1 : 6 x 10(10) M-circle dot, implies that this emission must come from a compact region <60 pc, possibly containing a second active galactic nucleus (AGN). The combined H-2 mass derived for both objects, using the [CI]2-1 emission, is 3 : 3 x 10(10) M-circle dot. The total CO(7-6)/[CI]2-1 line flux ratio of 0.2 suggests a low excitation molecular gas reservoir and / or enhanced atomic carbon in cosmic ray dominated regions. We detect spatially-resolved H2O 211 202 emission-for the first time in a high-z unlensed galaxy-near the outer radio lobe to the east, and near the bend of the radio jet to the west of the radio galaxy. No underlying 246 GHz continuum emission is seen at either position. We suggest that the H2O emission is excited in the cooling region behind slow (10-40 km s(-1)) shocks in dense molecular gas (10(3-5) cm(3)). The extended water emission is likely evidence of the radio jet's impact on cooling and forming molecules in the post-shocked gas in the halo and inter-cluster gas, similar to what is seen in low-z clusters and other high-z radio galaxies. These observations imply that the passage of the radio jet in the interstellar and inter-cluster medium not only heats gas to high temperatures, as is commonly assumed or found in simulations, but also induces cooling and dissipation, which can lead to substantial amounts of cold dense molecular gas. The formation of molecules and strong dissipation in the halo gas of MRC1138-262 may explain both the extended diffuse molecular gas and the young stars observed around MRC1138-262.

gas

proto-cluster

Astronomy & Astrophysics

star-formation

submillimeter galaxy

early universe

galaxies: high-redshift

h-alpha emitters

galaxies: ISM

galaxies: evolution

stephans quintet

high-redshift

radio galaxy mrc-1138-262

galaxies: active

molecular

Galaxy: halo

infrared galaxies

Författare

B. Gullberg

Max Planck-institutet

University of Durham

European Southern Observatory (ESO)

M. Lehnert

Université Pierre et Marie Curie (UPMC)

C. De Breuck

European Southern Observatory (ESO)

S. Branchu

Laboratoire d'Astrophysique de Bordeaux

European Southern Observatory (ESO)

H. Dannerbauer

Universität Wien

Guillaume Drouart

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

B. Emonts

Centro de Astrobiologia (CAB)

P. Guillard

Université Pierre et Marie Curie (UPMC)

N. Hatch

University of Nottingham

N. Nesvadba

Université Paris-Sud

A.A. Omont

Université Pierre et Marie Curie (UPMC)

N. Seymour

Curtin University

J. Vernet

European Southern Observatory (ESO)

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 591

Ämneskategorier

Astronomi, astrofysik och kosmologi

Fundament

Grundläggande vetenskaper

DOI

10.1051/0004-6361/201527647