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Selected: Q

Q 1208 + 1011 - The most distant imaged quasar, or a binary?

Astronomy and Astrophysics – Astrophysics
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Q values of models in the main-sequence band

Astronomy and Astrophysics – Astrophysics
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Q&A Peter Korevaar

Astronomy and Astrophysics – Astrophysics
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q-Deformation and Semidualisation in 3d Quantum Gravity

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
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q-Deformation of Lorentzian spin foam models

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
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q-deformed algebras $U_q(so_n)$ and their representations

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
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q-Deformed spin foam models of quantum gravity

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
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Q-LET - Quick Lensing Estimation Tool - An application to SN2003es

Astronomy and Astrophysics – Astrophysics
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Q-Phonon Approach for Low-Lying 1- Two-Phonon States in Spherical Nuclei

Astronomy and Astrophysics – Astrophysics
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Q-stars in scalar-tensor gravitational theories

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
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Q0045-3337: models including strong lensing by a spiral galaxy

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Q0353-383 - The best case yet for abundance anomalies in quasars

Astronomy and Astrophysics – Astrophysics
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Q0906+6930: The Highest-Redshift Blazar

Astronomy and Astrophysics – Astrophysics
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Q0957+561 - Detailed models of the gravitational lens effect

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Q0957+561 - Effects of random stars on the gravitational lens

Astronomy and Astrophysics – Astrophysics
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Q0957+561 revised: CO emission from a disk at z=1.4

Astronomy and Astrophysics – Astrophysics
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q1 Eri: a solar-type star with a planet and a dust belt

Astronomy and Astrophysics – Astrophysics
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Q1208+1011: Search for the lensing galaxy

Astronomy and Astrophysics – Astrophysics
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Q2122-444: a naked AGN fully dressed

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Q2237+0305 in X-rays: spectra and variability with XMM-Newton

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