Sub-arcsecond imaging of the water emission in Arp 220.

ABSTRACT:

Aims

Extragalactic observations of water emission can provide valuable insights into the excitation of the interstellar medium. In particular they allow us to investigate the excitation mechanisms in obscured nuclei, i.e. whether an active galactic nucleus or a starburst dominate.

Methods

We use sub-arcsecond 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 modelling of the water lines

SUBMITTER: Konig S 

PROVIDER: S-EPMC5687566 | biostudies-literature | 2017 Jun

REPOSITORIES: biostudies-literature