10.9k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
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12 papers · 2 filters
Unification of Spectral States of Accreting Black Holes
Juri Poutanen, Paolo Coppi
Several galactic black holes show transitions between spectral states. In this paper we present a unifying radiation transfer model that can fit the spectral data in both states. W…
An SPH code for galaxy formation problems; Presentation of the code
John Hultman, Daniel Kaellander
We present and test a code for two-fluid simulations of galaxy formation, one of the fluids being collision-less. The hydrodynamical evolution is solved through the SPH method whil…
Abundances in metal-rich stars - Detailed abundance analysis of 47 G and K dwarf stars with [Me/H] 0.10 dex
Sofia Feltzing, Bengt Gustafsson
We have derived elemental abundances of O, Na, Mg, Al, Si, Ca, Ti, Cr, Mn, Fe, Co, Ni for 47 G and K dwarf, with [Me/H]>0.1 dex. The selection of stars was based on their kinematic…
Near-infrared narrow-band photometry of M-giant and Mira stars: models meet observations
R. Alvarez, B. Plez
From near-infrared, narrow-band photometry of 256 oxygen-rich Mira variables we obtain evidence about the loops that these stars follow in colour-colour diagrams. We also find a ph…
Physical Characteristics of the Spectral States of Galactic Black Holes
Juri Poutanen, Julian H. Krolik, Felix Ryde
Using simple analytical estimates we show how the physical parameters characterizing different spectral states of the galactic black hole candidates can be determined using spectra…
The rise and fall of the NaMgAl stars
Jocelyn Tomkin, Bengt Edvardsson, David L. Lambert +1
We have made new abundance determinations for a sample of NaMgAl stars. These stars, which are a subgroup of the nearby metal-rich field F and G disk dwarfs, were first identified…
Two-phase spectral modelling of 1E1740.7-2942
O. Vilhu, J. Nevalainen, J. Poutanen +5
Combined ASCA and SIGMA data of 1E1740.7-2942 during the standard state (September 1993 and 1994) were fitted with two-phase models (ISMBB/Poutanen at al. and ADAF/Narayan et al.).…
50 TeV HEGRA Sources and Infrared Radiation
V. Berezinsky, Lars Bergström, H. R. Rubinstein
The recent observations of 50 TeV gamma radiation by HEGRA have the potential of determining the extragalactic flux of infrared radiation. The fact that radiation is observed in th…
A stellar endgame -- the born-again Sakurai's object
M. Asplund, B. Gustafsson, D. L. Lambert +1
The surface chemical composition of this remarkable star shows that it is hydrogen-deficient, carbon-rich and enriched in the light s-process elements. Spectra taken in May and Oct…
Brightness Dependent Properties of Gamma Ray Bursts
Boris Stern, Juri Poutanen, Roland Svensson
Brightness dependent correlations have been conclusively detected in the average time profiles of gamma-ray bursts (GRBs). Determining the time constants of the stretched exponenti…
Astrophysical-Neutrino Detection with Angular and Energy Resolution
L. Bergstrom, J. Edsjo, M. Kamionkowski
We investigate the improvement in sensitivity to astrophysical point sources of energetic ( GeV) neutrinos which can be achieved with angular and/or energy resolution of…
Two-phase pair corona model for AGN: physical modelling and diagnostics
Juri Poutanen, Roland Svensson, Boris Stern
The predictions of the two-phase accretion disc-corona models for active galactic nuclei are compared with observations. We discuss the possibility to use X-ray spectral slopes, eq…