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1. Full Text Wind properties of variable B supergiants: Evidence of pulsations connected with mass-loss episodes
by Haucke, M and Cidale, L.S and Venero, R.O.J and Curé, M and Kraus, M and Kanaan, S and Arcos, C
Astronomy and Astrophysics, ISSN 0004-6361, 06/2018, Volume 614, p. A91
Context. Variable B supergiants (BSGs) constitute a heterogeneous group of stars with complex photometric and spectroscopic behaviours. They exhibit mass-loss... 
Stars: winds, outflows | Stars: mass-loss | Stars: early-type | Supergiants | IUE MEGA CAMPAIGN | LOSS RATES | ALPHA-CYGNI VARIABLES | stars: winds, outflows | HOT LUMINOUS STARS | O-TYPE STARS | stars: early-type | EARLY-TYPE STARS | ASTRONOMY & ASTROPHYSICS | BLANKETED MODEL ATMOSPHERES | stars: mass-loss | supergiants | FUNDAMENTAL PARAMETERS | TERMINAL VELOCITIES | DRIVEN STELLAR WINDS
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2. Full Text NUMERICAL SIMULATION OF HOT ACCRETION FLOWS. III. REVISITING WIND PROPERTIES USING THE TRAJECTORY APPROACH
by Yuan, Feng and Gan, Zhaoming and Narayan, Ramesh and Sadowski, Aleksander and Bu, Defu and Bai, Xue-Ning
Astrophysical Journal, ISSN 0004-637X, 05/2015, Volume 804, Issue 2, pp. 101 - 12
Previous MHD simulations have shown that wind must exist in black hole hot accretion flows. In this paper, we continue our study by investigating the detailed... 
hydrodynamics | black hole physics | galaxies: jets | accretion, accretion disks | SAGITTARIUS-A | ADVECTION-DOMINATED ACCRETION | SPINNING BLACK-HOLE | 3-DIMENSIONAL MAGNETOHYDRODYNAMIC SIMULATIONS | ELLIPTIC GALAXIES | MASS OUTFLOWS | ACTIVE GALACTIC NUCLEI | ASTRONOMY & ASTROPHYSICS | 2-DIMENSIONAL MODELS | FEEDBACK | 2 DIMENSIONS | Stellar winds | Magnetohydrodynamics | Accretion | Computer simulation | Simulation | Flux | Outflow | Trajectories
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3. Full Text Atmospheres and wind properties of non-spherical AGB stars
by Liljegren, S and Höfner, S and Freytag, B and Bladh, S and Institutionen för fysik och astronomi and Teknisk-naturvetenskapliga vetenskapsområdet and Teoretisk astrofysik and Uppsala universitet and Fysiska sektionen
Astronomy and Astrophysics, ISSN 0004-6361, 11/2018, Volume 619, p. A47
Context. The wind-driving mechanism of asymptotic giant branch (AGB) stars is commonly attributed to a two-step process: first, gas in the stellar atmosphere... 
Shock waves | Stars: winds, outflows | Stars: AGB and post-AGB | Stars: atmospheres | Stars: oscillations | stars: atmospheres | CIRCUMSTELLAR DUST | SERIES | MIRA VARIABLES | stars: AGB and post-AGB | GRAINS | stars: oscillations | OUTFLOWS | ASTRONOMY & ASTROPHYSICS | stars: winds outflows | DYNAMIC-MODEL ATMOSPHERES | SHELLS | SIMULATIONS | SILICATE | shock waves | Stellar winds | Wind | Computer simulation | Gas dynamics | Atmospheric models | Luminosity | Boundary conditions | Wind models | Asymptotic giant branch stars | Convection | Lower atmosphere | Stellar atmospheres | Properties (attributes) | Shock fronts | Atmosphere | Astronomical models | Convection cells | Wind velocities | Stellar surfaces | Three dimensional models | Pulsation | Physics - Solar and Stellar Astrophysics | Astronomi med intiktning mot astrofysik | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy with specialization in Astrophysics | Astronomy, Astrophysics and Cosmology
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4. Full Text Physical parameters and wind properties of galactic early B supergiants
by Crowther, P.A and Lennon, D.J and Walborn, N.R
Astronomy and Astrophysics, ISSN 0004-6361, 01/2006, Volume 446, Issue 1, pp. 279 - 293
We present optical studies of the physical and wind properties, plus CNO chemical abundances, of 25 O9.5-B3 Galactic supergiants. We employ non-LTE, line... 
Stars: abundances | Stars: evolution | Stars: fundamental parameters | Stars: mass-loss | Stars: early-type | stars : early-type | SPECTROSCOPIC ANALYSIS | FAR-ULTRAVIOLET | stars : fundamental parameters | NLTE-MODELS | ASTRONOMY & ASTROPHYSICS | BLANKETED MODEL ATMOSPHERES | stars : evolution | MAGELLANIC-CLOUDS | STELLAR WINDS | MASS-LOSS | TERMINAL VELOCITIES | LOW METALLICITY ENVIRONMENT | OB-STARS | stars : mass-loss | stars : abundances | 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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5. Full Text The very slow solar wind: Properties, origin and variability
by Sanchez‐Diaz, Eduardo and Rouillard, Alexis P and Lavraud, Benoit and Segura, Kevin and Tao, Chihiro and Pinto, Rui and Sheeley, N. R and Plotnikov, Illya
Journal of Geophysical Research: Space Physics, ISSN 2169-9380, 04/2016, Volume 121, Issue 4, pp. 2830 - 2841
Solar wind slower than 300 km/s, hereafter termed very slow solar wind (VSSW), is seldom observed at 1 AU. It was, however, commonly measured inside 0.7 AU by... 
Helios | slow solar wind | heliospheric plasma sheet | helium abundance | SPEED | COROTATING STREAMS | CORONAL STREAMERS | HELIUM ABUNDANCE | HYDRODYNAMIC STREAMS | PLASMA | MAGNETIC-FIELDS | 1 AU | 3-DIMENSIONAL MODEL | ASTRONOMY & ASTROPHYSICS | CYCLE | Charged particles | Magnetic fields | Wind | Temperature | Magnetohydrodynamics | Variability | Proton density (concentration) | Fluid flow | Density | Wind speed | Variable structure | Laws | Collisions | Scaling laws | Modelling | Solar cycle | Solar wind | Fluctuations | Compressing | Computational fluid dynamics | Spacecraft | Solar maximum | Flux | Ions | Abundance | Helium ions | Helium | Velocity | Solar wind velocity | Solar activity | Mass flux | Photosphere | Scaling | Acceleration
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6. Full Text The VLT-FLAMES Tarantula Survey. XVII. Physical and wind properties of massive stars at the top of the main sequence
by Bestenlehner, J.M and Gräfener, G and Vink, J.S and Najarro, F and de Koter, A and Sana, H and Evans, C.J and Crowther, P.A and Hénault-Brunet, V and Herrero, A and Langer, N and Schneider, F.R.N and Simón-Díaz, S and Taylor, W.D and Walborn, N.R
Astronomy & Astrophysics, ISSN 0004-6361, 2014, Volume 570, p. A38
The evolution and fate of very massive stars (VMS) is tightly connected to their mass-loss properties. Their initial and final masses differ significantly as a... 
Stars: atmospheres | Stars: fundamental parameters | Stars: mass-loss | Stars: early-type | Stars: Wolf-Rayet | stars: atmospheres | SPECTRAL CLASSIFICATION | HOT LUMINOUS STARS | WOLF-RAYET STARS | O-TYPE STARS | NITROGEN LINE SPECTROSCOPY | 30 DORADUS | stars: Wolf-Rayet | stars: early-type | RADIATION-DRIVEN WINDS | ASTRONOMY & ASTROPHYSICS | BLANKETED MODEL ATMOSPHERES | stars: mass-loss | WN STARS | stars: fundamental parameters | LARGE-MAGELLANIC-CLOUD | Physics - Solar and Stellar Astrophysics
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7. Full Text AGE DEPENDENCE of WIND PROPERTIES for SOLAR-TYPE STARS: A 3D STUDY
by Réville, Victor and Folsom, Colin P and Strugarek, Antoine and Brun, Allan Sacha
Astrophysical Journal, ISSN 0004-637X, 12/2016, Volume 832, Issue 2, p. 145
Young and rapidly rotating stars are known for intense, dynamo-generated magnetic fields. Spectropolarimetric observations of those stars in precisely aged... 
stars: magnetic field | methods: numerical | stars: winds, outflows | magnetohydrodynamics (MHD) | stars: rotation | Sun: evolution | ANGULAR-MOMENTUM EVOLUTION | MASS-LOSS RATES | MODEL | DRIVEN | ASTRONOMY & ASTROPHYSICS | BRAKING | ACTIVITY-ROTATION RELATIONSHIP | STELLAR WINDS | MAGNETIC-FIELD | INTERACTION REGIONS | ACTIVE STARS | Physics - Solar and Stellar Astrophysics
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8. Full Text Pulsation-induced atmospheric dynamics in M-type AGB stars: Effects on wind properties, photometric variations and near-IR CO line profiles
by Liljegren, S and Höfner, S and Eriksson, K and Nowotny, W and Institutionen för fysik och astronomi and Teknisk-naturvetenskapliga vetenskapsområdet and Teoretisk astrofysik and Uppsala universitet and Fysiska sektionen
Astronomy and Astrophysics, ISSN 0004-6361, 10/2017, Volume 606, p. A6
Context. Wind-driving in asymptotic giant branch (AGB) stars is commonly attributed to a two-step process. First, matter in the stellar atmosphere is levitated... 
Stars: winds, outflows | Stars: AGB and post-AGB | Infrared: stars | Stars: atmospheres | Line: profiles | stars: atmospheres | SYNTHETIC PHOTOMETRY | CIRCUMSTELLAR DUST | infrared: stars | stars: AGB and post-AGB | LONG-PERIOD VARIABLES | stars: winds, outflows | VLTI/AMBER | CARBON-RICH MIRAS | OBSERVABLE PROPERTIES | GRAINS | EVOLUTION | line: profiles | ASTRONOMY & ASTROPHYSICS | GIANTS II | MODEL ATMOSPHERES | Physics - Solar and Stellar Astrophysics | Fysik | stars: winds | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | outflows | Natural Sciences | Astronomy, Astrophysics and Cosmology
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9. Full Text Early magnetic B-type stars: X-ray emission and wind properties
by Oskinova, L. M and Todt, H and Ignace, R and Brown, J. C and Cassinelli, J. P and Hamann, W.-R
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2011, Volume 416, Issue 2, pp. 1456 - 1474
We present a comprehensive study of X-ray emission by, and wind properties of, massive magnetic early B-type stars. Dedicated XMM-Newton observations were... 
X‐rays: stars | stars: massive | stars: magnetic field | stars: mass loss | techniques: spectroscopic | Stars: magnetic field | Stars: mass loss | X-rays: stars | Techniques: spectroscopic | Stars: massive | PHOTON IMAGING CAMERA | MASS-LOSS RATES | SLOWLY PULSATING-B | O-TYPE STARS | CHEMICALLY PECULIAR STARS | ASTRONOMY & ASTROPHYSICS | XMM-NEWTON OBSERVATIONS | DRIVEN STELLAR WINDS | SIGMA-ORI-E | HELIUM-STRONG STARS | THETA ORIONIS-C | Thermodynamics | Electronic mail systems | Ionization | Analysis | X-rays | Spectra | Magnetic fields | Astronomy | Astrophysics | X ray astronomy | Star & galaxy formation | Stars & galaxies | Physics - Solar and Stellar Astrophysics
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10. Full Text Solar Wind Properties During Juno's Approach to Jupiter: Data Analysis and Resulting Plasma Properties Utilizing a 1‐D Forward Model
by Wilson, R. J and Bagenal, Fran and Valek, Philip W and McComas, D. J and Allegrini, Frederic and Ebert, Robert W and Kim, Thomas K and Kurth, W. S and Szalay, Jamey R and Thomsen, Michelle F
Journal of Geophysical Research: Space Physics, ISSN 2169-9380, 04/2018, Volume 123, Issue 4, pp. 2772 - 2786
The Jovian Auroral Distributions Experiment ion sensor (JADE‐I) on board the National Aeronautics and Space Administration's Juno mission measured solar wind... 
solar | JADE | upstream | Juno | wind | BOW SHOCK | MISSION | DAWN FLANK | MAGNETOSPHERE | ASTRONOMY & ASTROPHYSICS | MAGNETOPAUSE | VOYAGER | MAGNETIC-FIELD | MAGNETOTAIL | Data analysis | Aeronautics | Magnetopause | Spacecraft | Jupiter atmosphere | Ram pressure | Magnetospheric ions | Magnetospheres | Magnetosphere | Jupiter | Space missions | Jupiter probes | Thermal plasmas | Solar wind properties | Solar wind | Magnetopause models | Solar wind ions
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11. Full Text Stellar and wind properties of massive stars in the central parsec of the Galaxy
by Martins, F and Genzel, R and Hillier, D.J and Eisenhauer, F and Paumard, T and Gillessen, S and Ott, T and Trippe, S
Astronomy and Astrophysics, ISSN 0004-6361, 06/2007, Volume 468, Issue 1, pp. 233 - 254
Context. How star formation proceeds in the Galactic Center is a debated question. Addressing this question will help us understand the origin of the cluster... 
Stars: winds, outflows | Stars: atmospheres | Stars: fundamental parameters | Stars: early-type | Galaxy: center | Stars: Wolf-Rayet | stars : atmospheres | EVOLUTIONARY STATUS | stars : early-type | stars : winds, outflows | ENIGMATIC WN8 STARS | stars : Wolf-Rayet | GALACTIC-HII-REGIONS | stars : fundamental parameters | WOLF-RAYET STARS | O-TYPE STARS | ASTRONOMY & ASTROPHYSICS | BLANKETED MODEL ATMOSPHERES | Galaxy : center | FUNDAMENTAL PARAMETERS | INFRARED SPECTROSCOPY | QUANTITATIVE SPECTROSCOPY | ARCHES CLUSTER | 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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12. Full Text Effects of anisotropic thermal conduction on wind properties in hot accretion flow
by Bu, De-Fu and Wu, Mao-Chun and Yuan, Ye-Fei
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2016, Volume 459, Issue 1, pp. 746 - 753
Previous works have clearly shown the existence of winds from black hole hot accretion flow and investigated their detailed properties. In extremely low... 
Conduction | Hydrodynamics | Accretion, accretion discs | Black hole physics | ADVECTION-DOMINATED ACCRETION | GRMHD SIMULATIONS | COLLISIONLESS PLASMA | hydrodynamics | MAGNETOTHERMAL INSTABILITY | accretion, accretion discs | 2 SPACE DIMENSIONS | black hole physics | ASTRONOMY & ASTROPHYSICS | conduction | BLACK-HOLE ACCRETION | MAGNETOROTATIONAL INSTABILITY | NUMERICAL-SIMULATION | RADIATION MAGNETOHYDRODYNAMICS CODE | ASTROPHYSICAL FLOWS | Wind | Effects | Anisotropy | Heat conductivity | Accretion disks | Astronomy | Physics - High Energy Astrophysical Phenomena
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