Issue |
A&A
Volume 587, March 2016
|
|
---|---|---|
Article Number | A15 | |
Number of page(s) | 11 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/201527457 | |
Published online | 12 February 2016 |
Evidence for a chemically differentiated outflow in Mrk 231⋆,⋆⋆
1
Department of Earth and Space SciencesChalmers University of Technology,
Onsala Observatory,
439 94
Onsala,
Sweden
e-mail:
johan.lindberg@nasa.gov
2
NASA Goddard Space Flight Center, Astrochemistry
Laboratory, Mail Code 691, 8800
Greenbelt Road, Greenbelt, MD
20771,
USA
3
Osservatorio di Radioastronomia (ORA-INAF), Italian ALMA Regional
Centre, c/o CNR, via Gobetti 101, 40129
Bologna,
Italy
4
Max-Planck-Institut für Radioastronomie,
Auf dem Hügel 69, 53121
Bonn,
Germany
5
Astronomy Department, King Abdulaziz University,
PO Box 80203, 21589
Jeddah, Saudi
Arabia
6
Leiden Observatory, Leiden University,
PO Box 9513, 2300 RA
Leiden, The
Netherlands
7
Observatorio Astronómico Nacional (OAN-IGN)-Observatorio de
Madrid, Alfonso XII,
3, 28014
Madrid,
Spain
8
Universidad de Alcalá de Henares, Departamento de Física, Campus
Universitario, 28871 Alcalá de
Henares, Madrid,
Spain
Received: 27 September 2015
Accepted: 14 December 2015
Aims. Our goal is to study the chemical composition of the outflows of active galactic nuclei and starburst galaxies.
Methods. We obtained high-resolution interferometric observations of HCN and HCO+J = 1 → 0 and J = 2 → 1 of the ultra-luminous infrared galaxy Mrk 231 with the IRAM Plateau de Bure Interferometer. We also use previously published observations of HCN and HCO+J = 1 → 0 and J = 3 → 2, and HNC J = 1 → 0 in the same source.
Results. In the line wings of the HCN, HCO+, and HNC emission, we find that these three molecular species exhibit features at distinct velocities which differ between the species. The features are not consistent with emission lines of other molecular species. Through radiative transfer modelling of the HCN and HCO+ outflow emission we find an average abundance ratio X(HCN) /X(HCO+) ≳ 1000. Assuming a clumpy outflow, modelling of the HCN and HCO+ emission produces strongly inconsistent outflow masses.
Conclusions. Both the anti-correlated outflow features of HCN and HCO+ and the different outflow masses calculated from the radiative transfer models of the HCN and HCO+ emission suggest that the outflow is chemically differentiated. The separation between HCN and HCO+ could be an indicator of shock fronts present in the outflow, since the HCN/HCO+ ratio is expected to be elevated in shocked regions. Our result shows that studies of the chemistry in large-scale galactic outflows can be used to better understand the physical properties of these outflows and their effects on the interstellar medium in the galaxy.
Key words: galaxies: individual: Mrk 231 / galaxies: active / galaxies: evolution / quasars: general / ISM: jets and outflows / ISM: molecules
Based on observations with the IRAM Plateau de Bure Interferometer. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain).
Reduced datacubes as FITS files are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/587/A15
© ESO, 2016
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.