A general study of the fermionic structure of the 331 models with eta arbitrary shows the possibility of obtaining 331 vector-like models with mirror fermions...
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Publicación331 vector-like models with mirror fermions as a possible solution for the discrepancy in the b-quark asymmetries, and for the neutrino mass and mixing pattern
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Publicación3C 279
IAUC 4739 available at Central Bureau for Astronomical Telegrams. IAUC 4739 available at Central Bureau for Astronomical Telegrams. IAUC 4739 available at...
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Publicación3C 279
IAUC 4798 available at Central Bureau for Astronomical Telegrams. IAUC 4798 available at Central Bureau for Astronomical Telegrams. IAUC 4798 available at...
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Publicación3C A Multi-Wavelength database for the future GTC cosmological surveys
The 3C Database aims to provide complete multi-wavelength information over different cosmological fields, such as GOODS, Groth or Sa68 allowing detailed studies...
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Publicación3D asymmetrical kinematics of mono-age populations from LAMOST and Gaia common red clump stars
With the LAMOST DR4 and Gaia DR2 common red clump giant stars, we investigate the three-dimensional kinematics of Milky Way disk stars in mono-age populations...
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Publicación3D MHD Simulations on Magnetic Flux Emergence
Not Available
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Publicación3D Models of Stellar Interactions
Symbiotic binaries consist of a cool, evolved mass-losing giant and an accreting compact companion. As symbiotic nebulae show similar morphologies to those in...
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Publicación3D non-LTE corrections for the 6Li/7Li isotopic ratio in solar-type stars
Doppler shifts induced by convective motions in stellar atmospheres affect the shape of spectral absorption lines and create slightly asymmetric line profiles...
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Publicación3D Optical and Radio Spectroscopy of Nearby LCBGs: NGC 7673, A Case Study
Luminous Compact Blue Galaxies (LCBGs) are high surface brightness starburst galaxies bluer than a typical SBc and with typical luminosities L*, which are...