Alkylnaphthalenes are not able to form Diels-Alder adducts with C70 fullerene but selected alkylnaphthalenes are able to yield weak charge-transfer complexes...
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PublicaciónC70 Fullerene charge-transfer interaction with alkylnaphthalenes, pinenes, and a diene
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PublicaciónCharge-transfer interaction between C60 fullerene and alkylnaphthalenes
A series of alkylnaphthalenes, namely 1,4-dimethylnaphthalene, 2,6-diethylnaphthalene, 2-ethylnaphthalene and pure naphthalene are not able to form Diels-Alder...
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PublicaciónEquinox in Petra: Land- and Skyscape in the Nabataean Capital
In earlier works, we had shown the actual possibility that the Nabataeans had used the Equinox, or an astronomical event equivalent to this, as an important...
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Publicación"Observations" of simulated dwarf galaxies. Star-formation histories from color-magnitude diagrams
Context. Apparent deviations between properties of dwarf galaxies from observations and simulations are known to exist, such as the "Missing Dwarfs" problem...
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Publicación'Global mapping' B-band photometry of a complete sample of Fornax and Virgo early-type galaxies
We present the B-band surface photometry of 19 early-type galaxies of the Virgo cluster, and of 28 galaxies of the same morphological type belonging to the...
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Publicación(596) Scheila in Outburst: A Probable Collision Event in the Main Asteroid Belt
Images of asteroid (596) Scheila have been acquired at various dates after the discovery of the 2010 outburst. Assuming a short-duration event scenario, as...
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Publicación(65) Cybele: detection of small silicate grains, water-ice, and organics
Context. (65) Cybele is the most representative member of a population of primitive asteroids in the outer edge of the main belt, the Cybele asteroids. Recent...
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Publicación(g -2 )<SUB>e ,μ</SUB> in an extended inverse type-III seesaw model
There has been a longstanding discrepancy between the experimental measurements of the electron and muon anomalous magnetic moments and their predicted values...
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Publicación(Re)Solving reionization with Lyα: how bright Lyα Emitters account for the z ≍ 2-8 cosmic ionizing background
The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV luminosity functions. Here, we introduce an emissivity framework based on...