Excitation and abundance of C3 in star forming cores Herschel/HIFI observations of the sight-lines to W31C and W49N
Artikel i vetenskaplig tidskrift, 2010
We present spectrally resolved observations of triatomic carbon (C-3) in several ro-vibrational transitions between the vibrational ground state and the low-energy nu(2) bending mode at frequencies between 1654-1897 GHz along the sight-lines to the submillimeter continuum sources W31C and W49N, using Herschel's HIFI instrument. We detect C-3 in absorption arising from the warm envelope surrounding the hot core, as indicated by the velocity peak position and shape of the line profile. The sensitivity does not allow to detect C-3 absorption due to diffuse foreground clouds. From the column densities of the rotational levels in the vibrational ground state probed by the absorption we derive a rotation temperature (T-rot) of similar to 50-70 K, which is a good measure of the kinetic temperature of the absorbing gas, as radiative transitions within the vibrational ground state are forbidden. It is also in good agreement with the dust temperatures for W31C and W49N. Applying the partition function correction based on the derived T-rot, we get column densities N(C-3) similar to 7-9 x 10(14) cm(-2) and abundance x(C-3) similar to 10(-8) with respect to H-2. For W31C, using a radiative transfer model including far-infrared pumping by the dust continuum and a temperature gradient within the source along the line of sight we find that a model with x(C-3) = 10(-8), T-kin = 30-50 K, N(C-3) = 1.5 x 10(15) cm(-2) fits the observations reasonably well and provides parameters in very good agreement with the simple excitation analysis.
ISM: individual objects: W31C
g10.6-0.4
dust
ISM: molecules
radiative transfer
individual objects: W49N
spiral-arm clouds
spectroscopy
translucent
irc+10216
interstellar c-3
hii-regions
ISM:
ISM: lines and bands
h-ii-regions
absorption
Författare
B. Mookerjea
Tata Institute of Fundamental Research
T. Giesen
Universität zu Köln
J. Stutzki
Universität zu Köln
J. Cernicharo
Centro de Astrobiologia (CAB)
J. R. Goicoechea
Centro de Astrobiologia (CAB)
M. de Luca
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
T. A. Bell
California Institute of Technology (Caltech)
H. Gupta
Jet Propulsion Laboratory, California Institute of Technology
M. Gerin
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
Carina Persson
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
P. Sonnentrucker
Johns Hopkins University
Z. Makai
Universität zu Köln
John H Black
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
F. Boulanger
Institut d'Astrophysique Spatiale
A. Coutens
Université de Toulouse
E. Dartois
Institut d'Astrophysique Spatiale
P. Encrenaz
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
E. Falgarone
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
T. R. Geballe
Gemini Observatory North
B. Godard
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
P. F. Goldsmith
Jet Propulsion Laboratory, California Institute of Technology
C. Gry
Laboratoire d'Astrophysique de Marseille
P. Hennebelle
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
E. Herbst
Ohio State University
P. Hily-Blant
Laboratoire d'Astrophysique de Grenoble
C. Joblin
Université de Toulouse
M. Kazmierczak
Uniwersytet Mikołaja Kopernika w Toruniu
R. Kolos
Polish Academy of Sciences
J. Krelowski
Uniwersytet Mikołaja Kopernika w Toruniu
D. C. Lis
California Institute of Technology (Caltech)
J. Martin-Pintado
Centro de Astrobiologia (CAB)
K. M. Menten
Max-Planck-Gesellschaft
Raquel Monje
California Institute of Technology (Caltech)
J. C. Pearson
Jet Propulsion Laboratory, California Institute of Technology
M. Perault
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
T. G. Phillips
California Institute of Technology (Caltech)
R. Plume
University of Calgary
M. Salez
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
S. Schlemmer
Universität zu Köln
M. Schmidt
Polish Academy of Sciences
D. Teyssier
European Space Astronomy Centre (ESAC)
C. Vastel
Université de Toulouse
S. Yu
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
P. Dieleman
Netherlands Institute for Space Research (SRON)
R. Güsten
Max-Planck-Gesellschaft
C. E. Honingh
Universität zu Köln
P. Morris
California Institute of Technology (Caltech)
P. Roelfsema
Netherlands Institute for Space Research (SRON)
R. Schieder
Universität zu Köln
Aggm Tielens
Universiteit Leiden
J. Zmuidzinas
California Institute of Technology (Caltech)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 521 1 Article Number: L13 - L13Ämneskategorier
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/201015095