Abstract
Etude des raies d'emission larges emanant de nuages formes par l'interaction d'un ecoulement de masse du noyau et d'un vent du disque dans le contexte d'un modele de quasar. Les rapports des raies et les profils des raies spectrales sont compatibles avec les observations
Sign-in/Register to access full text options 
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.
