tipa -- 9/10/2009

The relation between the most-massive star and its parental star cluster mass

  • Authors: C. Weidner (1,2), P. Kroupa (3), I. Bonnell (1) ((1) St Andrews University, (2) Pontificia Universidad Catolica de Chile, (3) AIfA Bonn)

The Extragalactic Background Light Absorption Feature in the Blazar Component of the Extragalactic Gamma-ray Background

The earliest stars and their relics in the Milky Way

Parameter Estimation from Improved Measurements of the CMB from QUaD

Relativistic Rayleigh-Taylor Instability of a Decelerating Shell and its Implications for Gamma Ray Bursts

Modeling the light curve of the transient SCP06F6

The influence of short term variations in AM CVn systems on LISA measurements

The impact of a strongly first-order phase transition on the abundance of thermal relics

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