Wednesday, February 16, 2005


Motl et al. calculate the integrated SZE effect for a sample of theoretical clusters with different assumed baryonic physics. They show that the integrated SZE provides a very accurate estimate of the mass.

Yao and Wang detect NeIX, OVII, and OVIII absorption lines in Chandra spectra of XRBs and use these to study the large-scale hot interstellar medium of the Galaxy.

Quirrenbach summarizes current technological progress on space-based coronographic imaging to find planets.

Keywords: clusters, ISM, planets

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