activity
19942013
most citedA Comptonization Model for Phase Lag Variability in GRS 1915+105

57 citations · 212 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2013★ 24 cited

Pulse profiles from thermally emitting neutron stars

R. Turolla, L. Nobili

The problem of computing the pulse profiles from thermally emitting spots on the surface of a neutron star in general relativity is reconsidered. We show that it is possible to ext…

astro-ph2002★ 21 cited

Power-law Tails from Dynamical Comptonization in Converging Flows

Roberto Turolla, Silvia Zane, Lev Titarchuk

The effects of bulk motion comptonization on the spectral formation in a converging flow onto a black hole are investigated. The problem is tackled by means of both a fully relativ…

astro-ph2000

Spectra of thermally unstable slim discs

Ewa Szuszkiewicz, Roberto Turolla, Luca Zampieri

Thermal instability driven by radiation pressure might be relevant for intrinsically bright accreting sources. The most promising candidate where this instability seems to be at wo…

astro-ph2000★ 57 cited

A Comptonization Model for Phase Lag Variability in GRS 1915+105

L. Nobili, R. Turolla, L. Zampieri +1

In this Letter we propose a simple thermal comptonization model to account for the observed properties of the phase lags associated to the ``plateau'' intervals of GRS 1915+105. By…

astro-ph2000

An efficient algorithm for two-dimensional radiative transfer in axisymmetric circumstellar envelopes and disks

C. P. Dullemond, R. Turolla

We present an algorithm for two-dimensional radiative transfer in axisymmetric, circumstellar media. The formal integration of the transfer equation is performed by a generalizatio…

astro-ph1996★ 29 cited

Time--dependent analysis of spherical accretion onto black holes

Luca Zampieri, John C. Miller, Roberto Turolla

Results are presented from a time--dependent, numerical investigation of spherical accretion onto black holes, within the framework of relativistic radiation hydrodynamics. We have…