Works matching IS 20754434 AND DT 2017 AND VI 5 AND IP 3
Results: 28
Upper Limits to Magnetic Fields in the Outskirts of Galaxies.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 55, doi. 10.3390/galaxies5030055
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Modeling Polarized Emission from Black Hole Jets: Application to M87 Core Jet.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 54, doi. 10.3390/galaxies5030054
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Dust Deficiency in the Interacting Galaxy NGC 3077.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 53, doi. 10.3390/galaxies5030053
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SALT Spectropolarimetry and Self-Consistent SED and Polarization Modeling of Blazars.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 52, doi. 10.3390/galaxies5030052
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A Non-Polynomial Gravity Formulation for Loop Quantum Cosmology Bounce.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 51, doi. 10.3390/galaxies5030051
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Knots in Relativistic Transverse Stratified Jets.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 50, doi. 10.3390/galaxies5030050
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The Outer Halos of Very Massive Galaxies: BCGs and their DSC in the Magneticum Simulations.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 49, doi. 10.3390/galaxies5030049
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Revisiting the Globular Cluster Systems of NGC3258 and NGC3268.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 48, doi. 10.3390/galaxies5030048
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Can CMB Surveys Help the AGN Community?
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 47, doi. 10.3390/galaxies5030047
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Globular Clusters and the Halos of Dwarf Galaxies.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 46, doi. 10.3390/galaxies5030046
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The HI Distribution Observed toward a Halo Region of the Milky Way.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 45, doi. 10.3390/galaxies5030045
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Disk Heating, Galactoseismology, and the Formation of Stellar Halos.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 44, doi. 10.3390/galaxies5030044
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Better Galactic Mass Models through Chemistry.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 43, doi. 10.3390/galaxies5030043
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The Baryonic Halos of Isolated Elliptical Galaxies.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 42, doi. 10.3390/galaxies5030042
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On the Kinematics, Stability and Lifetime of Kinematically Distinct Cores: A Case Study.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 41, doi. 10.3390/galaxies5030041
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Resolving the Extended Stellar Halos of Nearby Galaxies: The Wide-Field PISCeS Survey.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 40, doi. 10.3390/galaxies5030040
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Deep MOS Spectroscopy of NGC1316 Globular Clusters.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 39, doi. 10.3390/galaxies5030039
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The Brazil-Argentina Gemini Group for the Study of Globular Cluster Systems (BAGGs GCs): FLAMINGOS-2 and GMOS Data for NGC 1395.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 38, doi. 10.3390/galaxies5030038
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One Piece at a Time--Adding to the Puzzle of S0 Formation.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 37, doi. 10.3390/galaxies5030037
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How Clumpy Star Formation Affects Globular Cluster Systems.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 36, doi. 10.3390/galaxies5030036
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Distribution and Evolution of Metals in the Magneticum Simulations.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 35, doi. 10.3390/galaxies5030035
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Galaxies with Shells in the Illustris Simulation: Metallicity Signatures.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 34, doi. 10.3390/galaxies5030034
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The "Building Blocks" of Stellar Halos.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 33, doi. 10.3390/galaxies5030033
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High-Energy Polarization: Scientific Potential and Model Predictions.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 32, doi. 10.3390/galaxies5030032
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A Photometric Study of Giant Ellipticals and Their Stellar HalosWith VST.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 31, doi. 10.3390/galaxies5030031
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The Globular Cluster System of the Galaxy NGC 6876.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 30, doi. 10.3390/galaxies5030030
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The Extended Baryonic Halo of NGC 3923.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 29, doi. 10.3390/galaxies5030029
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Interstellar Reddening Effect on the Age Dating of Population II Stars.
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- Galaxies (2075-4434), 2017, v. 5, n. 3, p. 28, doi. 10.3390/galaxies5030028
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