Figure 1 from Revolutionizing Our Understanding of AGN Feedback and its Importance to Galaxy Evolution in the Era of the Next Generation Very Large Array

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Revolutionizing Our Understanding of AGN Feedback and its Importance to Galaxy Evolution in the Era of the Next Generation Very Large Array

Authors: K. Nyland, J. J. Harwood, D. D. Mukherjee, P. Jagannathan, W. Rujopakarn, B. Emonts, K. Alatalo, G. V. Bicknell, T. A. Davis, J. E. Greene, A. Kimball, M. Lacy, Carol Lonsdale, Colin Lonsdale, W. P. Maksym, D. C. Molnár, L. Morabito, E. J. Murphy, P. Patil, I. Prandoni, M. Sargent, and C. Vlahakis

2018 The Astrophysical Journal 859 23.

Provider: AAS Journals

Caption: Figure 1.

Antenna locations in the ngVLA configuration considered in this study. Major U.S. highways are shown in red. The array is centered on the compact core of the current VLA in New Mexico, and the additional antennas at intermediate and long baselines take into account local geography, land ownership, and infrastructure. The longest baselines of 513 km extend in the north-south direction into Mexico and will maximize the utility of the ngVLA for Galactic center studies.

Other Images in This Article

Copyright and Terms & Conditions