12 citations · 18 across the 6 of their papers we have counts for
6 papers
Turbulence and the characteristics of circumstellar discs
R. Riaz, D. R. G. Schleicher, S. Vanaverbeke +2
We investigate the properties of circumstellar discs (CDs) produced in hydrodynamical simulations of gravoturbulent core collapse considering Kolmogorov and Burger-type turbulence.…
Impact of radiation backgrounds on the formation of massive black holes
V. B. Díaz, D. R. G. Schleicher, S. Bovino +4
The presence of supermassive black holes (SMBHs) of a few billion solar masses at very high redshift has motivated us to study how these massive objects formed during the first bil…
Star formation at high redshift
P. Fibla, S. Bovino, R. Riaz +4
We present here a three-dimesional hydrodynamical simulation for star formation. Our aim is to explore the effect of the metal-line cooling on the thermodynamics of the star-format…
Episodic accretion in binary protostars emerging from self-gravitating solar mass cores
R. Riaz, S. Vanaverbeke, D. R. G. Schleicher
Observations show a large spread in the luminosities of young protostars, which are frequently explained in the context of episodic accretion. We here test this scenario using nume…
On the thermal sensitivity of binary formation in collapsing molecular clouds
R. Riaz, S. Z. Farooqui, S. Vanaverbeke
We report the results of a numerical study on the initial formation stages of low-mass protostellar binary systems. We determine the separation of protostellar binaries formed as a…
The early phase of multiple proto-stellar system emerged from collapse of molecular cloud under various initial thermal states
Rafil Riaz, Suhail Zaki Farooqui, Siegfried Vanaverbeke
An attempt is made here to revisit structure formation in a proto-stellar cloud during the early phase of evolution. Molecular cloud subjected to a set of various initial condition…