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Chapter and Conference Paper
Low-Mass Objects and the Dark Matter in the Halo
If the unseen matter in our Galaxy is provided by very low-mass star-like objects, we show that the halo infrared luminosity is dominated by 0. 1M ⊙ objects. In this case, the halo IMF must be muc...
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Chapter and Conference Paper
The light curve of SN 1987 A
We use a semi-analytical model of supernova light curves that extends Arnett's scheme [1,2] to include the effect of recombination of hydrogen, helium and heavy elements in the expanding ejecta. Introducing in...
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Chapter
Influence Of Quark Nuggets on Primordial Nucleosynthesis
There are many indications that the baryonic content of the universe is rather low. The observation of the luminous matter in galaxies leads to a ratio Ωbof the baryon density over the critical density of about 0...
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Chapter
Light Curves of Exploding Wolf-Rayet Stars
The removal of the extended hydrogen envelope surrounding the dense core of preexplosive stars by stellar winds or mass transfer onto a companion star, obviously, has consequences on the optical manifestation ...