Water abundance variations around high-mass protostars: HIFI observations of the DR21 region
Artikel i vetenskaplig tidskrift, 2010

Context. Water is a key molecule in the star formation process, but its spatial distribution in star-forming regions is not well known. Aims. We study the distribution of dust continuum and H2O and (CO)-C-13 line emission in DR21, a luminous star-forming region with a powerful outflow and a compact H II region. Methods. Herschel-HIFI spectra near 1100 GHz show narrow (CO)-C-13 10-9 emission and H2O 1(11)-0(00) absorption from the dense core and broad emission from the outflow in both lines. The H2O line also shows absorption by a foreground cloud known from ground-based observations of low-J CO lines. Results. The dust continuum emission is extended over 36 '' FWHM, while the (CO)-C-13 and H2O lines are confined to approximate to 24 '' or less. The foreground absorption appears to peak further North than the other components. Radiative transfer models indicate very low abundances of similar to 2 x 10(-10) for H2O and similar to 8 x 10(-7) for (CO)-C-13 in the dense core, and higher H2O abundances of similar to 4 x 10(-9) in the foreground cloud and similar to 7 x 10(-7) in the outflow. Conclusions. The high H2O abundance in the warm outflow is probably due to the evaporation of water-rich icy grain mantles, while the H2O abundance is kept down by freeze-out in the dense core and by photodissociation in the foreground cloud.

h-2

monte-carlo method

ISM: individual

line emission

objects: DR21

stars: formation

evolution

young stars

radiative-transfer

ISM: molecules

star-formation

excitation

absorption

cygnus-x

astrochemistry

Författare

F. F. S. van der Tak

Rijksuniversiteit Groningen

Netherlands Institute for Space Research (SRON)

M. G. Marseille

Netherlands Institute for Space Research (SRON)

F. Herpin

Laboratoire d'Astrophysique de Bordeaux

F. Wyrowski

Netherlands Institute for Space Research (SRON)

A. Baudry

Laboratoire d'Astrophysique de Bordeaux

S. Bontemps

Laboratoire d'Astrophysique de Bordeaux

J. Braine

Laboratoire d'Astrophysique de Bordeaux

S. Doty

Denison University

W. Frieswijk

Rijksuniversiteit Groningen

G. J. Melnick

Harvard-Smithsonian Center for Astrophysics

R. Shipman

Netherlands Institute for Space Research (SRON)

E. F. van Dishoeck

Universiteit Leiden

MPI fur Extraterrestrische Physik

A. O. Benz

Eidgenössische Technische Hochschule Zürich (ETH)

P. Caselli

University of Leeds

M. Hogerheijde

Universiteit Leiden

D. Johnstone

National Research Council Canada

University of Victoria

René Liseau

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

R. Bachiller

Observatorio Astronómico Nacional (OAN)

M. Benedettini

Istituto di Fisica dello Spazio Interplanetario, Rome

E. A. Bergin

University of Michigan

Per Bjerkeli

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

G. A. Blake

California Institute of Technology (Caltech)

S. Bruderer

Eidgenössische Technische Hochschule Zürich (ETH)

J. Cernicharo

Centro de Astrobiologia (CAB)

C. Codella

Istituto di Fisica dello Spazio Interplanetario, Rome

F. Daniel

Centro de Astrobiologia (CAB)

Observatoire de Paris-Meudon

A. M. di Giorgio

Istituto di Fisica dello Spazio Interplanetario, Rome

C. Dominik

Universiteit Van Amsterdam

P. Encrenaz

LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres

M. Fich

University of Waterloo

A. Fuente

Observatorio Astronómico Nacional (OAN)

T. Giannini

Istituto di Fisica dello Spazio Interplanetario, Rome

J. R. Goicoechea

Centro de Astrobiologia (CAB)

T. de Graauw

Atacama Large Millimeter-submillimeter Array (ALMA)

F. Helmich

Netherlands Institute for Space Research (SRON)

G. J. Herczeg

MPI fur Extraterrestrische Physik

J. K. Jorgensen

Köpenhamns universitet

L. Kristensen

Universiteit Leiden

B. Larsson

Stockholms universitet

D. Lis

California Institute of Technology (Caltech)

C. McCoey

University of Waterloo

D. A. Neufeld

Johns Hopkins University

B. Nisini

Istituto di Fisica dello Spazio Interplanetario, Rome

Michael Olberg

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

B. Parise

Universität zu Köln

Max-Planck-Gesellschaft

J. C. Pearson

California Institute of Technology (Caltech)

R. Plume

University of Calgary

C. Risacher

Netherlands Institute for Space Research (SRON)

J. Santiago

Observatorio Astronómico Nacional (OAN)

P. Saraceno

Istituto di Fisica dello Spazio Interplanetario, Rome

M. Tafalla

Observatorio Astronómico Nacional (OAN)

T. A. van Kempen

Harvard-Smithsonian Center for Astrophysics

R. Visser

Universiteit Leiden

S. F. Wampfler

Eidgenössische Technische Hochschule Zürich (ETH)

U. A. Yildiz

Universiteit Leiden

L. Ravera

Université de Toulouse

P. Roelfsema

Netherlands Institute for Space Research (SRON)

O. Siebertz

Universität zu Köln

D. Teyssier

Europeiska rymdorganisationen (ESA)

Astronomy and Astrophysics

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

Vol. 518 Article Number: L107 L107

Ämneskategorier (SSIF 2011)

Astronomi, astrofysik och kosmologi

DOI

10.1051/0004-6361/201014515

Mer information

Senast uppdaterat

2025-04-23