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20032019
most citedThe minimum mass for star formation, and the origin of binary brown dwarfs

162 citations · 989 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2019★ 16 cited

ALMA reveals a pseudo-disc in a proto-brown dwarf

B. Riaz, M. N. Machida, D. Stamatellos

We present the observational evidence of a pseudo-disc around the proto-brown dwarf Mayrit 1701117, the driving source of the large-scale HH~1165 jet. Our analysis is based on ALMA…

astro-ph.SR2012★ 9 cited

Revised analysis of SPIRE observations for 2M1207

B. Riaz, G. Lodato, D. Stamatellos +1

We have revised our analysis of the SPIRE observations of 2MASSW J1207334-393254 (2M1207). Recent PACS observations show a bright source located ~25" east of 2M1207. There are issu…

astro-ph.SR2011★ 57 cited

Disc Frequencies for Brown Dwarfs in the Upper Scorpius OB Association: Implications for Brown Dwarf Formation Theories

B. Riaz, N. Lodieu, S. Goodwin +2

We have investigated the brown dwarf (BD) and stellar disc fractions in the Upper Scorpius OB Association (USco) and compared them with several other young regions. We have compile…

astro-ph.GA2011★ 1 cited

Episodic accretion, radiative feedback, and their role in low-mass star formation

Dimitris Stamatellos, David Hubber, Anthony Whitworth

It is speculated that the accretion of material onto young protostars is episodic. We present a computational method to include the effects of episodic accretion in radiation hydro…

astro-ph.EP2011★ 133 cited

A natural formation scenario for misaligned and short-period eccentric extrasolar planets

Ingo Thies, Pavel Kroupa, Simon P. Goodwin +2

Recent discoveries of strongly misaligned transiting exoplanets pose a challenge to the established planet formation theory which assumes planetary systems to form and evolve in is…

astro-ph.GA2011★ 15 cited

The initial conditions of high-mass star formation: radiative transfer models of IRDCs seen in the Herschel Hi-GAL survey

L. A. Wilcock, J. M. Kirk, D. Stamatellos +13

The densest infrared dark clouds (IRDCs) may represent the earliest observable stage of high-mass star formation. These clouds are very cold, hence they emit mainly at far-infrared…