Abstract
On a effectue un balayage en continuum proche de 1,4 Ghz avec la configuration D du VLA centree sur l'amas Hercules de galaxies (A 2151). On donne les positions et les flux pour 65 sources 21-25 sources sont associees a des galaxies (principalement des galaxies brillantes) et la separation entre les positions radio et optique est ≤S 11 dans la plupart des cas
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
