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19962004
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Showing 1997Show all

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astro-ph1997

Microlensing results and the galactic models

F. De Paolis, Ph. Jetzer, G. Ingrosso

Microlensing results towards the LMC strongly depend on the properties of both the luminous and the dark matter distribution in the Galaxy. The two main sources of uncertainty come…

gr-qc1997

On the Stability of Real Scalar Boson Stars

Philippe Jetzer, David Scialom

We discuss spherically symmetric static solutions of the Einstein-Klein-Gordon equations for a real scalar field with a mass and a quartic self-interaction term. As for the massles…

astro-ph1997

Gravitational microlensing research

Philippe Jetzer

One of the most important problems in astrophysics concerns the nature of the dark matter in galactic halos, whose presence is implied mainly by the observed flat rotation curves i…

astro-ph1997

X-ray emission from dark clusters of MACHOs

F. De Paolis, G. Ingrosso, Ph. Jetzer +1

MACHOs (Massive Astrophysical Compact Halo Objects) - as discovered by microlensing experiments towards the LMC - provide a natural explanation for the galactic halo dark matter. A…

astro-ph1997

Microlensing implications for halo dark matter

F. De Paolis, Ph. Jetzer, G. Ingrosso +1

The observations of microlensing events in the Large Magellanic Cloud suggest that a sizable fraction ( 50%) of the galactic halo is in the form of MACHOs (Massive Astrophysi…

astro-ph1997

Baryonic Dark Matter

F. De Paolis, Ph. Jetzer, G. Ingrosso +1

Reasons supporting the idea that most of the dark matter in galaxies and clusters of galaxies is baryonic are discussed. Moreover, it is argued that most of the dark matter in gala…