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/index.php/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/index.php/ictp-saifr/1464
BibTex
@misc{ scivideos_SAIFR:1464, doi = {}, url = {https://scivideos.org/index.php/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/index.php/ictp-saifr/1464}} }
Rodrigo Nemmen
Talk numberSAIFR:1464
Source RepositoryICTP – SAIFR
Talk Type
Conference
Subject