Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (4 of 5)
APA
(2018). Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (4 of 5). ICTP South American Institute for Fundamental Research. https://scivideos.org/index.php/ictp-saifr/1467
MLA
Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (4 of 5). ICTP South American Institute for Fundamental Research, Dec. 06, 2018, https://scivideos.org/index.php/ictp-saifr/1467
BibTex
@misc{ scivideos_SAIFR:1467, doi = {}, url = {https://scivideos.org/index.php/ictp-saifr/1467}, author = {}, keywords = {ICTP-SAIFR, IFT, UNESP}, language = {en}, title = {Black Hole (g)astrophysics Modeling of extreme mass ratio in spirals (4 of 5)}, publisher = { ICTP South American Institute for Fundamental Research}, year = {2018}, month = {dec}, note = {SAIFR:1467 see, \url{https://scivideos.org/index.php/ictp-saifr/1467}} }
Rodrigo Nemmen
Talk numberSAIFR:1467
Source RepositoryICTP – SAIFR
Talk Type
Conference
Subject