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19982026
most citedStellar and total baryon mass fractions in groups and clusters since redshift 1

328 citations · 2.1k across the 184 of their papers we have counts for

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Showing 2006Show all

6 papers · 1 filter

astro-ph2006★ 23 cited

The Structure of the Inner HH 34 Jet from Optical Integral Field Spectroscopy

Tracy L. Beck, A. Riera, A. C. Raga +1

We present high spatial resolution optical integral field spectroscopy of a collimated Herbig-Haro jet viewed nearly edge-on. Maps of the line emission, velocity centroid, and velo…

astro-ph2006

O VI and H_2 Lines in Sunspots

Nicolas Labrosse, Huw Morgan, Shadia Rifai Habbal +1

Sunspots are locations on the Sun where unique atmospheric conditions prevail. In particular, the very low temperatures found above sunspots allow the emission of H_2 lines. In thi…

astro-ph2006

SK 1: A Possible Case of Triggered Star Formation in Perseus

M. Rengel, K. Hodapp, J. Eisloeffel

According to a triggered star formation scenario (e.g. Martin-Pintado & Cernicharo 1987) outflows powered by young stellar objects shape the molecular clouds, can dig cavities, and…

astro-ph2006★ 36 cited

The role of the energy equation in the fragmentation of protostellar discs during stellar encounters

G. Lodato, F. Meru, C. Clarke +1

In this paper, we use high-resolution smoothed particle hydrodynamics (SPH) simulations to investigate the response of a marginally stable self-gravitating protostellar disc to a c…

astro-ph2006★ 21 cited

Boltzmann moment equation approach for the numerical study of anisotropic stellar disks

E. I. Vorobyov, Ch. Theis

We present the Boltzmann moment equation approach for the dynamics of stars (BEADS-2D), which is a finite-difference Eulerian numerical code designed for the modelling of anisotrop…

astro-ph2006★ 96 cited

Optical and infrared observations of the Type IIP SN2002hh from day 3 to 397

M. Pozzo, W. P. S. Meikle, J. T. Rayner +6

We present optical and infrared (IR) observations of the type IIP SN2002hh from 3 to 397 days after explosion. The optical spectroscopic (4-397d) and photometric (3-278d) data are…