Titlebook: Nuclear Dynamics: From Quarks to Nuclei; Proceedings of the X M. Teresa Pe?a,Alfred Stadler,Ji?í Adam Conference proceedings 2003 Springer-

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W. Plessasatter from a low mass star is transferred to its neutron star companion. As a class, these sources are characterized by a level of X-ray emission ranging from about 10. to 10. ergs s. (corresponding to mass accretion rates onto the neutron star of about 10. to 10. M⊙ yr.). For a detailed review of t

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Franz Grossbe launched in December 2001. IRS will provide SIRTF with low and moderate-spectral resolution spectroscopic capabilities from 5.3. to 40.. The IRS instrument has no moving parts (the so called ‘bolt-and-go’ philosophy) and it is composed of four separate modules, with two of the modules providing R

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J. C. Caillon,J. Labarsouquee Universe, differ from the nearby ones. .New observational windows at ultraviolet, infrared and millimetricwavelengths (provided by ROSAT, IRAM, IUE, IRAS, ISO) have revealedthat galaxies contain a wealth of components: very hot gas, atomichydrogen, molecules, dust, dark matter. A significant advan

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J.-M. Lagetbe launched in December 2001. IRS will provide SIRTF with low and moderate-spectral resolution spectroscopic capabilities from 5.3. to 40.. The IRS instrument has no moving parts (the so called ‘bolt-and-go’ philosophy) and it is composed of four separate modules, with two of the modules providing R

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