activity
19962026
most citedDetection of titanium oxide in the atmosphere of a hot Jupiter

194 citations · 3.7k across the 152 of their papers we have counts for

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Showing 1998Show all

8 papers · 1 filter

astro-ph1998

Three-dimensional SPH simulations of accretion discs

Henri M. J. Boffin, Kei Haraguchi, Takuya Matsuda

We discuss some 3D numerical simulations of accretion discs using the SPH method and a polytropic equation of state. We show that discs exist even for as large value of the polytro…

astro-ph1998★ 28 cited

The structure of young star clusters

P. P. Gladwin, S. Kitsionas, H. M. J. Boffin +1

We analyse and compare the clustering of young stars in Chamaeleon I and Taurus. We compute the mean surface-density of companion stars \bar{N} as a function of angular displacemen…

astro-ph1998★ 4 cited

Spiral Structure in IP Peg: Confronting Theory and Observations

Takuya Matsuda, Makoto Makita, Hiroshi Yukawa +1

The first convincing piece of evidence of spiral structure in the accretion disc in IP Pegasi was found by Steeghs et al. (1997). We performed two kinds of 2D hydrodynamic simulati…

astro-ph1998★ 47 cited

Numerical simulations of protostellar encounters III. Non-coplanar disc-disc encounters

S. J. Watkins, A. S. Bhattal, H. M. J. Boffin +2

It is expected that an average protostar will undergo at least one impulsive interaction with a neighbouring protostar whilst a large fraction of its mass is still in a massive, ex…

astro-ph1998★ 42 cited

Numerical simulations of protostellar encounters II. Coplanar disc-disc encounters

S. J. Watkins, A. S. Bhattal, H. M. J. Boffin +2

It is expected that an average protostar will undergo at least one impulsive interaction with a neighbouring protostar whilst a large fraction of its mass is still in a massive, ex…

astro-ph1998★ 71 cited

Numerical simulations of protostellar encounters I. Star-disc encounters

H. M. J. Boffin, S. J. Watkins, A. S. Bhattal +2

It appears that most stars are born in clusters, and that at birth most stars have circumstellar discs which are comparable in size to the separations between the stars. Interactio…

astro-ph1998★ 1 cited

Numerical Computation of Two Dimensional Wind Accretion of Isothermal Gas

Eiji Shima, Takuya Matsuda, Ulrich Anzer +2

A new numerical algorithm for calculating isothermal wind accretion flows has been developed and is applied here to the analysis of the hydrodynamics of two-dimensional plane symme…

astro-ph1998★ 36 cited

Gas-cooling by dust during dynamical fragmentation

A. P. Whitworth, H. M. J. Boffin, N. Francis

We suggest that the abrupt switch, from hierarchical clustering on scales larger than 0.04 pc, to binary (and occasionally higher multiple) systems on smaller scales, which Larson…