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1. Full Text Atmospheric NLTE-models for the spectroscopic analysis of blue stars with winds - II. Line-blanketed models
by Puls, J and Urbaneja, M.A and Venero, R and Repolust, T and Springmann, U and Jokuthy, A and Mokiem, M.R
Astronomy & Astrophysics, ISSN 0004-6361, 2005, Volume 435, Issue 2, pp. 669 - 698
We present new or improved methods for calculating NLTE, line-blanketed model atmospheres for hot stars with winds ( spectral types A to O), with particular... 
Line: formation | Stars: atmospheres | Stars: massloss | Stars: early-type | Methods: numerical | stars : atmospheres | MASSIVE STARS | stars : early-type | line : formation | HOT LUMINOUS STARS | O-TYPE STARS | SOBOLEV APPROXIMATION | LAMBDA-ITERATION METHOD | RADIATION-DRIVEN WINDS | B-TYPE SUPERGIANTS | ASTRONOMY & ASTROPHYSICS | methods : numerical | MAGELLANIC-CLOUDS | STELLAR WINDS | EFFECTIVE TEMPERATURE SCALE | stars : mass-loss | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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2. Full Text Role of f(R, T, Rμ νTμ ν) model on the stability of cylindrical stellar model
by Yousaf, Z and Bhatti, M. Zaeem-ul-Haq and Farwa, Ume
European Physical Journal C, ISSN 1434-6044, 06/2017, Volume 77, Issue 6, pp. 1 - 13
The aim of this paper is to investigate the stable/unstable regimes of the non-static anisotropic filamentary stellar models in the framework of f (R, T, R mu... 
GRAVITATIONAL COLLAPSE | FILAMENTS | SPHERICAL COLLAPSE | DYNAMICAL INSTABILITY | STARS | OSCILLATIONS | SUPERNOVAE | UNIVERSE | MODIFIED GRAVITY | LAMBDA | PHYSICS, PARTICLES & FIELDS | Formulations | Conservation laws | Gravitation | Adiabatic flow | Stability | Perturbation methods | Astronomical models | Stability analysis | Stellar models | Physics - General Physics | Nuclear and particle physics. Atomic energy. Radioactivity | Astrophysics
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3. Full Text Rotating massive main-sequence stars. I. Grids of evolutionary models and isochrones
by Brott, I.|info:eu-repo/dai/nl/304829811 and de Mink, S.E.|info:eu-repo/dai/nl/304833231 and Cantiello, M.|info:eu-repo/dai/nl/304840866 and Langer, N.|info:eu-repo/dai/nl/304829498 and de Koter, A and Evans, C.J and Hunter, I and Trundle, C and Vink, J.S.|info:eu-repo/dai/nl/212372971
Astronomy and Astrophysics, ISSN 0004-6361, 2011, Volume 530, Issue A115, p. A115
We present a dense grid of evolutionary tracks and isochrones of rotating massive main-sequence stars. We provide three grids with different initial... 
Stars: abundances | Stars: evolution | Stars: early-type | Stars: massive | Stars: rotation | PRESUPERNOVA EVOLUTION | stars: evolution | B-TYPE STARS | ECLIPSING BINARIES | CHEMICAL-COMPOSITIONS | stars: abundances | GAMMA-RAY BURSTS | DIFFERENTIAL ROTATION | VLT-FLAMES SURVEY | stars: early-type | STELLAR EVOLUTION | ASTRONOMY & ASTROPHYSICS | stars: massive | LARGE-MAGELLANIC-CLOUD | stars: rotation | ATMOSPHERIC PARAMETERS | Physics - Solar and Stellar Astrophysics
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4. Full Text Consistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs
by Woitke, P and Min, M and Pinte, C and Thi, W. -F and Kamp, I and Rab, C and Anthonioz, F and Antonellini, S and Baldovin-Saavea, C and Carmona, A and Dominik, C and Dionatos, O and Greaves, J and Güdel, M and Ilee, J. D and Liebhart, A and Ménard, F and Rigon, L and Waters, L. B. F. M and Aresu, G and Meijerink, R and Spaans, M
Astronomy and Astrophysics, ISSN 0004-6361, 2016, Volume 586, Issue February 2016, p. A103
We propose a set of standard assumptions for the modelling of Class II and III protoplanetary disks, which includes detailed continuum radiative transfer,... 
Line: formation | Circumstellar matter | Astrochemistry | Radiative transfer | Stars: formation | Methods: numerical | radiative transfer | MAIN-SEQUENCE STARS | FINAL ARCHIVE SPECTRA | methods: numerical | YOUNG STELLAR OBJECTS | stars: formation | RADIATION THERMOCHEMICAL MODELS | line: formation | SPECTRAL ENERGY-DISTRIBUTIONS | circumstellar matter | TRANSIENTLY HEATED PARTICLES | ASTRONOMY & ASTROPHYSICS | RO-VIBRATIONAL EMISSION | CIRCUMSTELLAR DISKS | T-TAURI STARS | HERBIG AE/BE STARS | astrochemistry | Dust | Polycyclic aromatic hydrocarbons | Planet formation | Settling | Continuums | Disks | Opacity
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5. Full Text The STAGGER-grid: A grid of 3D stellar atmosphere models I. Methods and general properties
by Magic, Z and Collet, R and Asplund, M and Trampedach, R and Hayek, W and Chiavassa, A and Stein, RF and Nordlund, A
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 09/2013, Volume 557, pp. A26 - np
Aims. We present the Stagger-grid, a comprehensive grid of time-dependent, three-dimensional (3D), hydrodynamic model atmospheres for late-type stars with... 
stars: atmospheres | COOL DWARF STARS | SOLAR GRANULATION | radiative transfer | SURFACE CONVECTION | METAL-POOR STARS | hydrodynamics | MIXING-LENGTH | stars: abundances | convection | 3-DIMENSIONAL HYDRODYNAMICAL SIMULATIONS | ASTRONOMY & ASTROPHYSICS | CHEMICAL-COMPOSITION | stars: fundamental parameters | RED GIANT STARS | RADIAL OSCILLATIONS | SPECTRAL-LINE FORMATION | Stellar atmospheres | Searching | Stars | Astronomical models | Hydrodynamics | Mathematical models | Radiative transfer | Three dimensional models | Physics - Solar and Stellar Astrophysics
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6. Full Text Testing lowered isothermal models with direct N-body simulations of globular clusters – II. Multimass models
by Peuten, M and Zocchi, A and Gieles, M and Hénault-Brunet, V
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 470, Issue 3, pp. 2736 - 2761
Lowered isothermal models, such as the multimass Michie-King models, have been successful in describing observational data of globular clusters. In this study,... 
Stars: black holes | Globular clusters: general | Stars: kinematics and dynamics | Galaxies: star clusters: general | Methods: numerical | ENERGY EQUIPARTITION | stars: black holes | STAR-CLUSTERS | INDIVIDUAL STARS | SEGREGATION | methods: numerical | STELLAR-SYSTEMS | PRIMORDIAL BINARIES | EVOLUTION | globular clusters: general | PHOTOELECTRIC RADIAL-VELOCITIES | ASTRONOMY & ASTROPHYSICS | MASS FUNCTION | stars: kinematics and dynamics | DYNAMICAL MODELS | galaxies: star clusters: general | Physics - Astrophysics of Galaxies
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7. Full Text The Stagger-grid: A grid of 3D stellar atmosphere models III. The relation to mixing length convection theory
by Magic, Z and Weiss, A and Asplund, M
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 01/2015, Volume 573, p. A89
Aims. We investigate the relation between 1D atmosphere models that rely on the mixing length theory and models based on full 3D radiative hydrodynamic (RHD)... 
stars: atmospheres | SOLAR GRANULATION | stars: evolution | SURFACE CONVECTION | hydrodynamics | MAIN-SEQUENCE | SUN | convection | stars: solar-type | GENERAL-PROPERTIES | stars: late-type | ENVELOPES | ASTRONOMY & ASTROPHYSICS | STARS | TURBULENT CONVECTION | NUMERICAL SIMULATIONS | HYDRODYNAMICAL MODELS | Envelopes | Stellar atmospheres | Atmospheric models | Convection modes | Constants | Mathematical models | Entropy | Three dimensional models | Physics - Solar and Stellar Astrophysics
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8. Full Text Evolution of asymptotic giant branch stars: II. Optical to far-infrared isochrones with improved TP-AGB models
by Marigo, P and Girardi, L and Bressan, A and Groenewegen, M.A.T and Silva, L and Granato, G.L
Astronomy and Astrophysics, ISSN 0004-6361, 05/2008, Volume 482, Issue 3, pp. 883 - 905
We present a large set of theoretical isochrones, whose distinctive features mostly reside on the greatly-improved treatment of the thermally-pulsing... 
Astronomical data bases: miscellaneous | Stars: evolution | Galaxies: Magellanic Clouds | Stars: AGB and post-AGB | Stars: Hertzsprung-Russell (HR) and C-M diagrams | Stars: carbon | COLOR-MAGNITUDE DIAGRAMS | astronomical data bases : miscellaneous | SINGLE STELLAR POPULATIONS | stars : carbon | MASS-LOSS RATES | LONG-PERIOD VARIABLES | POPULATION SYNTHESIS MODELS | galaxies : Magellanic Clouds | stars : Hertzsprung-Russell (HR) and C-M diagrams | stars : AGB and post-AGB | DUST CONDENSATION SEQUENCE | ACTIVE GALACTIC NUCLEI | DA WHITE-DWARFS | ASTRONOMY & ASTROPHYSICS | stars : evolution | SPITZER-SPACE-TELESCOPE | LARGE-MAGELLANIC-CLOUD | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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9. Full Text Comparing star formation models with interferometric observations of the protostar NGC 1333 IRAS 4A: I. Magnetohydrodynamic collapse models
by Frau, P and Galli, D and Girart, J.M
Astronomy and Astrophysics, ISSN 0004-6361, 2011, Volume 535, p. A44
Context. Observations of dust polarized emission toward star forming regions trace the magnetic field component in the plane of the sky and provide constraints... 
Magnetohydrodynamics (MHD) | ISM: individual objects: NGC 1333 IRAS 4A | Polarization | Stars: formation | ISM: magnetic fields | SINGULAR ISOTHERMAL TOROIDS | ROTATION | GRAVITATIONAL COLLAPSE | OUTFLOW | POLARIZED DUST EMISSION | stars: formation | EVOLUTION | ASTRONOMY & ASTROPHYSICS | LINE | MOLECULAR CLOUD CORES | polarization | MAGNETIC-FIELD | magnetohydrodynamics (MHD) | NGC-1333 IRAS-4
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10. Full Text Mesa isochrones and stellar tracks (MIST). I. solar-scaled models
by Choi, Jieun and Dotter, Aaron and Conroy, Charlie and Cantiello, Matteo and Paxton, Bill and Johnson, Benjamin D
Astrophysical Journal, ISSN 0004-637X, 06/2016, Volume 823, Issue 2, pp. 102 - 102
This is the first of a series of papers presenting the Modules for Experiments in Stellar Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project, a... 
stars: general | stars: interiors | stars: evolution | ANGULAR-MOMENTUM TRANSPORT | LOW-MASS STARS | B-TYPE STARS | METAL-POOR STARS | ASYMPTOTIC GIANT BRANCH | PRE-MAIN-SEQUENCE | GAMMA-RAY BURSTS | ASTRONOMY & ASTROPHYSICS | HERTZSPRUNG-RUSSELL DIAGRAM | LARGE-MAGELLANIC-CLOUD | M-CIRCLE-DOT | Mesas | Websites | Constraint modelling | Evolution | Stellar evolution | Combustion | Carbon | Age | Physics - Solar and Stellar Astrophysics
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11. Full Text The Galactic WN stars Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation
by Hamann, W.-R and Gräfener, G and Liermann, A
Astronomy and Astrophysics, ISSN 0004-6361, 10/2006, Volume 457, Issue 3, pp. 1015 - 1031
Context. Very massive stars pass through the Wolf-Rayet (WR) stage before they finally explode. Details of their evolution have not yet been safely... 
Stars: evolution | Stars: winds, outflows | Stars: atmospheres | Stars: mass-loss | Stars: early-type | Stars: Wolf-Rayet | stars : atmospheres | TAILORED ANALYSES | stars : early-type | stars : winds, outflows | LOSS RATES | stars : Wolf-Rayet | BINARY | POLARIZATION VARIABILITY | WOLF-RAYET STARS | SPECTROSCOPY | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | stars : evolution | FUNDAMENTAL PARAMETERS | CLUSTER | stars : mass-loss | LOW-MASS COMPANION | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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