Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (5 of 5)
APA
(2018). Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (5 of 5). ICTP South American Institute for Fundamental Research. https://scivideos.org/index.php/ictp-saifr/1473
MLA
Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (5 of 5). ICTP South American Institute for Fundamental Research, Dec. 07, 2018, https://scivideos.org/index.php/ictp-saifr/1473
BibTex
@misc{ scivideos_SAIFR:1473, doi = {}, url = {https://scivideos.org/index.php/ictp-saifr/1473}, author = {}, keywords = {ICTP-SAIFR, IFT, UNESP}, language = {en}, title = {Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (5 of 5)}, publisher = { ICTP South American Institute for Fundamental Research}, year = {2018}, month = {dec}, note = {SAIFR:1473 see, \url{https://scivideos.org/index.php/ictp-saifr/1473}} }
Rodrigo Nemmen
Talk numberSAIFR:1473
Source RepositoryICTP – SAIFR
Talk Type
Conference
Subject