Subarcsecond imaging of the water emission in Arp 220
Artikel i vetenskaplig tidskrift, 2017
Aims. Extragalactic observations of water emission can provide valuable insight into the excitation of the interstellar medium. In particular they allow us to investigate the excitation mechanisms in obscured nuclei, that is, whether an active galactic nucleus or a starburst dominates.
Methods. We use subarcsecond resolution observations to tackle the nature of the water emission in Arp 220. ALMA Band 5 science verification observations of the 183 GHz H2O 313 − 220 line, in conjunction with new ALMA Band 7 H2O 515 − 422 data at 325 GHz, and supplementary 22 GHz H2O 616 − 523 VLA observations, are used to better constrain the parameter space in the excitation modeling of the water lines.
Results. We detect 183 GHz H2O and 325 GHz water emission toward the two compact nuclei at the center of Arp 220, being brighter in Arp 220 West. The emission at these two frequencies is compared to previous single-dish data and does not show evidence of variability. The 183 and 325 GHz lines show similar spectra and kinematics, but the 22 GHz profile is significantly different in both nuclei due to a blend with an NH3 absorption line.
Conclusions. Our findings suggest that the most likely scenario to cause the observed water emission in Arp 220 is a large number of independent masers originating from numerous star-forming regions.
galaxies: individual: Arp 220 / galaxies: ISM / galaxies: starburst / ISM: molecules
Författare
Sabine König
Astronomi och plasmafysik
S. Martín
Atacama Large Millimeter-submillimeter Array
European Southern Observatory Santiago
Sebastien Muller
Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium
Jose Cernicharo
CSIC - Instituto de Ciencia de Materiales de Madrid (ICMM)
K. Sakamoto
Institute of Astrophysics and Astronomy, Academia Sinica Taiwan
Laura Zschaechner
Max Planck Institut fur Astronomie
E. M. Humphreys
European Southern Observatory
Tony Mroczkowski
European Southern Observatory
Melanie Krips
IRAM Institut de RadioAstronomie Millimetrique
Maud Galametz
CEA Saclay
European Southern Observatory
Susanne Aalto
Astronomi och plasmafysik
Wouter Vlemmings
Astronomi och plasmafysik
Jürgen Ott
National Radio Astronomy Observatory Socorro
D. S. Meier
New Mexico Institute of Mining and Technology
A. Fuente
Observatorio Astronomico Nacional
S. G. Burillo
OAN
Roberto Neri
IRAM Institut de RadioAstronomie Millimetrique
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 602 42- 30331Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Fundament
Grundläggande vetenskaper
DOI
10.1051/0004-6361/201630331