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pro vyhledávání: '"Goicovic, Felipe G."'
Autor:
Nogueira, Pedro Henrique, Zurlo, Alice, Pérez, Sebastián, González-Ruilova, Camilo, Cieza, Lucas A., Hales, Antonio, Bhowmik, Trisha, Ruíz-Rodríguez, Dary A., Principe, David A., Herczeg, Gregory J., Williams, Jonathan P., Cuadra, Jorge, Montesinos, Matías, Cuello, Nicolás, Chavan, Prachi, Casassus, Simon, Zhu, Zhaohuan, Goicovic, Felipe G.
Episodic accretion is a low-mass pre-main sequence phenomenon characterized by sudden outbursts of enhanced accretion. These objects are classified into two: protostars with elevated levels of accretion that lasts for decades or more, called FUors, a
Externí odkaz:
http://arxiv.org/abs/2305.15647
When a star approaches a black hole closely, it may be pulled apart by gravitational forces in a tidal disruption event (TDE). The flares produced by TDEs are unique tracers of otherwise quiescent supermassive black holes (SMBHs) located at the centr
Externí odkaz:
http://arxiv.org/abs/1902.08202
Massive black hole binaries (MBHBs) represent an unavoidable outcome of hierarchical galaxy formation, but their dynamical evolution at sub-parsec scales is poorly understood, due to a combination of uncertainties in theoretical models and lack of fi
Externí odkaz:
http://arxiv.org/abs/1801.06179
Autor:
Goicovic, Felipe G., Maureira-Fredes, Cristian, Sesana, Alberto, Amaro-Seoane, Pau, Cuadra, Jorge
In currently favoured hierarchical cosmologies, the formation of massive black hole binaries (MBHBs) following galaxy mergers is unavoidable. Still, due the complex physics governing the (hydro)dynamics of the post-merger dense environment of stars a
Externí odkaz:
http://arxiv.org/abs/1801.04937
The formation of massive black hole binaries (MBHBs) is an unavoidable outcome of galaxy evolution via successive mergers. However, the mechanism that drives their orbital evolution from parsec separations down to the gravitational wave (GW) dominate
Externí odkaz:
http://arxiv.org/abs/1602.01966
We model numerically the evolution of $10^4M_\odot$ turbulent molecular clouds in near-radial infall onto $10^6M_\odot$, equal-mass super-massive black hole binaries, using a modified version of the SPH code GADGET-3. We investigate the different gas
Externí odkaz:
http://arxiv.org/abs/1501.04012
Autor:
Goicovic, Felipe G.1, Cuadra, Jorge1, Sesana, Alberto2, Meiron, Y., Li, S., Liu, F.-K., Spurzem, R.
Publikováno v:
Proceedings of the International Astronomical Union. Aug2014 Supplement, Vol. 10 Issue S312, p48-51. 4p.
Akademický článek
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Hydrodynamical moving-mesh simulations of the tidal disruption of stars by supermassive black holes.
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Jul2019, Vol. 487 Issue 1, p981-992, 12p
Autor:
Goicovic, Felipe G, Maureira-Fredes, Cristián, Sesana, Alberto, Amaro-Seoane, Pau, Cuadra, Jorge
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 9/21/2018, Vol. 479 Issue 3, p3438-3455, 18p