SAIFR:1464

Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (3 of 5)

APA

(2018). Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (3 of 5). ICTP South American Institute for Fundamental Research. https://scivideos.org/ictp-saifr/1464

MLA

Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (3 of 5). ICTP South American Institute for Fundamental Research, Dec. 05, 2018, https://scivideos.org/ictp-saifr/1464

BibTex

          @misc{ scivideos_SAIFR:1464,
            doi = {},
            url = {https://scivideos.org/ictp-saifr/1464},
            author = {},
            keywords = {ICTP-SAIFR, IFT, UNESP},
            language = {en},
            title = {Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (3 of 5)},
            publisher = { ICTP South American Institute for Fundamental Research},
            year = {2018},
            month = {dec},
            note = {SAIFR:1464 see, \url{https://scivideos.org/ictp-saifr/1464}}
          }
          
Rodrigo Nemmen
Talk numberSAIFR:1464
Talk Type Conference
Subject