Aims: Several primitive families in the inner region of the main asteroid belt were identified as potential sources for two near-Earth asteroids (NEAs), (101955...
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PublicaciónThe last pieces of the primitive inner belt puzzle: Klio, Chaldaea, Chimaera, and Svea
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PublicaciónThe Lazy Giants: APOGEE Abundances Reveal Low Star Formation Efficiencies in the Magellanic Clouds
We report the first APOGEE metallicities and α-element abundances measured for 3600 red giant stars spanning a large radial range of both the Large (LMC) and...
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PublicaciónThe lens SW05 J143454.4+522850: a fossil group at redshift 0.6?
Fossil groups are considered the end product of natural galaxy group evolution in which group members sink towards the centre of the gravitational potential due...
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PublicaciónThe Leonid Outburst of 1996
There is strong anticipation that the Leonid meteor shower could produce storm-level activity in 1998 and/or 1999. The well-documented Leonid outburst in 1996...
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PublicaciónThe Li I resonance line in the spectra of X-ray nova accretion discs
We study the formation of the Li I lambda 6708 Angstroms resonance doublet in spectra of X-ray novae during the stage of outburst decay. We discuss the general...
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PublicaciónThe Liège Oscillation code
The Liège Oscillation code can be used as a stand-alone program or as a library of subroutines that the user calls from a Fortran main program of his own to...
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PublicaciónThe limit of mass for gravitational collapse and nuclear forces at short distance
On the basis of the current knowledge about the size of the neutron, the nucleon-nucleon interaction, and the limit on the ratio Gm/c2R < 4/9 imposed by General...
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PublicaciónThe Limited Influence of Pressure Gradients on Late-Type Stellar Line Asymmetries
Line asymmetries and shifts are powerful tools for studying velocity fields in the stellar photospheres. Other effects, however, could also generate asymmetries...
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PublicaciónThe Line Emission Region in III Zw 2: Kinematics and Variability
We have studied the Lyα, Hβ, Hα, and Mg II λ2798 line profiles of the Seyfert 1 galaxy III Zw 2. The shapes of these broad emission lines show evidence of a...