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
Subscribe to:
Post Comments (Atom)
No comments:
Post a Comment