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1. Full Text Chemodynamical evolution of the Milky Way disk: II. Variations with Galactic radius and height above the disk plane
by Minchev, I and Chiappini, C and Martig, M
Astronomy and Astrophysics, ISSN 0004-6361, 12/2014, Volume 572, pp. A92 - 19
In the first paper of this series (Paper I) we presented a new approach for studying the chemodynamical evolution in disk galaxies, focusing on the Milky Way.... 
Galaxy: evolution | Galaxies: evolution | Galaxy: disk | Galaxy: formation | Galaxy: kinematics and dynamics | Galaxy: abundances | DENSITY WAVES | galaxies: evolution | SPIRAL GALAXIES | CHEMICAL EVOLUTION | MONO-ABUNDANCE SUBPOPULATIONS | MINOR MERGERS | THICK DISC | SOLAR NEIGHBORHOOD | ASTRONOMY & ASTROPHYSICS | VELOCITY STREAMS | METALLICITY GRADIENT | SPECTROSCOPIC SURVEY | Populations | Planes | Heating | Galactic evolution | Migration | Milky Way Galaxy | Disks | Astronomy
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2. Full Text Water and interstellar complex organics associated with the HH 212 protostellar disc: On disc atmospheres, disc winds, and accretion shocks
by Codella, C and Bianchi, E and Tabone, B and Lee, C.-F and Cabrit, S and Ceccarelli, C and Podio, L and Bacciotti, F and Bachiller, R and Chapillon, E and Gueth, F and Gusdorf, A and Lefloch, B and Leurini, S and Pineau Des Forêts, G and Rygl, K.L.J and Tafalla, M
Astronomy and Astrophysics, ISSN 0004-6361, 09/2018, Volume 617, p. A10
Context. The unprecedented combination of high-sensitivity and high angular resolution provided by the ALMA interferometer allows us to shed light on the... 
ISM: jets and outflows | ISM: molecules | Stars: formation | ISM: individual objects: HH212 | stars: formation | JET HH-212 | ENVELOPES | OUTFLOW | SUBMILLIMETER | ASTRONOMY & ASTROPHYSICS | GAS | MOLECULES
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3. Full Text DISK FORMATION VERSUS DISK ACCRETION - WHAT POWERS TIDAL DISRUPTION EVENTS?
by Piran, Tsvi and Svirski, Gilad and Krolik, Julian and Cheng, Roseanne M and Shiokawa, Hotaka
Astrophysical Journal, ISSN 0004-637X, 06/2015, Volume 806, Issue 2, pp. 164 - 8
A tidal disruption event (TDE) takes place when a star passes near enough to a massive black hole to be disrupted. About half the star's matter is given... 
black hole physics | stars: black holes | galaxies: nuclei | accretion, accretion disks | FLARES | STELLAR DISRUPTION | PS1-10JH | BULGES | SUPERMASSIVE BLACK-HOLE | STAR | ASTRONOMY & ASTROPHYSICS | GALACTIC NUCLEI | GALAXIES | SIMULATIONS | FLOWS | Accretion | Heating | Luminosity | Black holes (astronomy) | Nuclear power generation | Formations | Disruption | Accretion disks
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4. Full Text Exploring the Milky Way stellar disk : A detailed elemental abundance study of 714 F and G dwarf stars in the solar neighbourhood
by Bensby, T and Feltzing, S and Oey, M.S
Astronomy and Astrophysics, ISSN 0004-6361, 02/2014, Volume 562, pp. A71 - np
Aims. The aim of this paper is to explore and map the age and abundance structure of the stars in the nearby Galactic disk. Methods. We have conducted a... 
Galaxy: evolution | Stars: abundances | Galaxy: disk | Stars: fundamental parameters | Stars: kinematics and dynamics | Galaxy: formation | NEARBY STARS | METAL-RICH STARS | ECHELLE SPECTROGRAPH | K-GIANTS | stars: abundances | THICK DISK | LINE-DATA-BASE | ASTRONOMY & ASTROPHYSICS | AGE-METALLICITY RELATION | MODEL ATMOSPHERES | stars: fundamental parameters | stars: kinematics and dynamics | GENEVA-COPENHAGEN SURVEY | GALACTIC CHEMICAL EVOLUTION | Subgiant stars | Orbitals | Aluminum | Stars | Solar neighborhood | Abundance | Disks | Dwarf stars | Physics - Astrophysics of Galaxies | Fysik | Astronomi, astrofysik och kosmologi | Physical Sciences | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
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5. Full Text Forming disc galaxies in major mergers - III. the effect of angular momentum on the radial density profiles of disc galaxies
by Peschken, N and Athanassoula, E and Rodionov, S.A
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2017, Volume 468, Issue 1, pp. 994 - 1004
We study the effect of angular momentum on the surface density profiles of disc galaxies, using high-resolution simulations of major mergers whose remnants... 
Galaxies: spiral | Galaxies: structure | Galaxies: kinematics and dynamics | SURFACE-BRIGHTNESS PROFILES | OUTER DISKS | SPIRAL GALAXIES | STAR-FORMATION | galaxies: structure | EXPONENTIAL DISKS | EVOLUTION | SPITZER SURVEY | ASTRONOMY & ASTROPHYSICS | STELLAR STRUCTURE | BARRED GALAXIES | galaxies: kinematics and dynamics | galaxies: spiral | PARTICLE HYDRODYNAMICS SIMULATIONS | Physics - Astrophysics of Galaxies | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics
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6. Full Text Non-axisymmetric line-driven disc winds - I. Disc perturbations
by Dyda, Sergei and Proga, Daniel
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2018, Volume 475, Issue 3, pp. 3786 - 3796
We study mass outflows driven from accretion discs by radiation pressure due to spectral lines. To investigate non-axisymmetric effects, we use the ATHENA++... 
Hydrodynamics | Cataclysmic variables | Stars: winds | Novae | Methods: numerical | Outflows | hydrodynamics | methods: numerical | stars: winds, outflows | ACCRETION DISKS | novae, cataclysmic variables | CONSTRAINED TRANSPORT | INSTABILITIES | DIMENSIONS | UNSPLIT GODUNOV METHOD | ACTIVE GALACTIC NUCLEI | MODELS | IDEAL MHD | ASTRONOMY & ASTROPHYSICS | STARS | STELLAR WINDS | Stellar winds | Wind | Axisymmetric | Accretion | Radiation | Perturbation | Fluxes | Accretion disks | Radiation pressure | Time dependence | Emissivity | Outflow | Line spectra | Kinetic energy | Deposition | Physics - High Energy Astrophysical Phenomena
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7. Full Text Chemodynamical evolution of the milky Way disk: I. the solar vicinity
by Minchev, I and Chiappini, C and Martig, M
Astronomy and Astrophysics, ISSN 0004-6361, 2013, Volume 558, pp. A9 - np
In the first paper of this series, we present a new approach for studying the chemo-dynamical evolution in disk galaxies, which consists of fusing disk... 
Galaxy: evolution | Galaxies: evolution | Galaxy: formation | Galaxy: kinematics and dynamics | Galaxy: abundances | Solar neighborhood | METALLICITY DISTRIBUTION | galaxies: evolution | METAL-RICH STARS | CHEMICAL EVOLUTION | THICK DISK | KINEMATIC PROPERTIES | MINOR MERGERS | ASTRONOMY & ASTROPHYSICS | solar neighborhood | GALACTIC ABUNDANCE GRADIENT | GALAXY FORMATION | RADIAL MIGRATION | PARTICLE HYDRODYNAMICS SIMULATIONS | Enrichment | Computer simulation | Astronomical models | Milky Way Galaxy | Disks | Evolution | Mathematical models | Chemical evolution
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8. Full Text The epoch of disk settling: Z ∼ 1 to now
by Kassin, Susan A and Weiner, Benjamin J and Faber, S.M and Gardner, Jonathan P and Willmer, C.N.A and Coil, Alison L and Cooper, Michael C and Devriendt, Julien and Dutton, Aaron A and Guhathakurta, Puragra and Koo, David C and Metevier, A.J and Noeske, Kai G and Primack, Joel R
Astrophysical Journal, ISSN 0004-637X, 10/2012, Volume 758, Issue 2, pp. 106 - 14
We present evidence from a sample of 544 galaxies from the DEEP2 Survey for evolution of the internal kinematics of blue galaxies with stellar masses ranging... 
galaxies: formation | galaxies: fundamental parameters | galaxies: kinematics and dynamics | galaxies: evolution | Spectral emissivity | Galaxies | Galactic evolution | Settling | Kinematics | Disk galaxies | Universe | Inclination | Physics - Cosmology and Nongalactic Astrophysics | ROTATION | RED SHIFT | VELOCITY | ENERGY SPECTRA | GALACTIC EVOLUTION | POTENTIALS | PHOTON EMISSION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTRONOMY | ASTROPHYSICS | INCLINATION | MASS | STARS | GALAXIES | UNIVERSE
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9. Full Text Disc reflection and a possible disc wind during a soft X-ray state in the neutron star low-mass X-ray binary 1RXS J180408.9-342058
by Degenaar, N and Altamirano, D and Parker, M and Miller-Jones, J.C.A and Miller, J.M and Heinke, C.O and Wijnands, R and Ludlam, R and Parikh, A and Hessels, J.W.T and Gusinskaia, N and Deller, A.T and Fabian, A.C
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2016, Volume 461, Issue 4, pp. 4049 - 4058
1RXS J180408.9-342058 is a transient neutron star low-mass X-ray binary that exhibited a bright accretion outburst in 2015. We present NuSTAR, Swift, and... 
342058 | Stars: winds, outflows | Stars:neutron | X-rays: binaries | Accretion, accretion discs | Stars: individual: 1RXS J180408.9 | CLUSTER NGC 6652 | COMPTON-HEATED WINDS | stars: winds, outflows | accretion, accretion discs | stars: neutron | ORBITAL PERIOD | stars: individual: 1RXS J180408.9-342058 | ACTIVE GALACTIC NUCLEI | ACCRETION DISC | BLACK-HOLE CANDIDATE | ASTRONOMY & ASTROPHYSICS | TRANSMISSION GRATING SPECTROMETER | PULSAR SAX J1808.4-3658 | XMM-NEWTON OBSERVATIONS | BROAD-BAND SPECTRUM | Physics - High Energy Astrophysical Phenomena
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10. Full Text The Gaia -ESO Survey: Separating disk chemical substructures with cluster models∗: Evidence of a separate evolution in the metal-poor thin disk
by Rojas-Arriagada, A and Recio-Blanco, A and De Laverny, P and Schultheis, M and Guiglion, G and Mikolaitis, S and Kordopatis, G and Hill, V and Gilmore, G and Randich, S and Alfaro, E.J and Bensby, T and Koposov, S.E and Costado, M.T and Franciosini, E and Hourihane, A and Jofré, P and Lardo, C and Lewis, J and Lind, K and Magrini, L and Monaco, L and Morbidelli, L and Sacco, G.G and Worley, C.C and Zaggia, S and Chiappini, C and Institutionen för fysik och astronomi and Teknisk-naturvetenskapliga vetenskapsområdet and Observationell astrofysik and Uppsala universitet and Fysiska sektionen
Astronomy and Astrophysics, ISSN 0004-6361, 02/2016, Volume 586
Context. Recent spectroscopic surveys have begun to explore the Galactic disk system on the basis of large data samples, with spatial distributions sampling... 
Galaxy: stellar content | Stars: abundances | Galaxy: formation | Galaxy: abundances | MILKY-WAY DISK | GALACTIC THICK | NEARBY STARS | stars: abundances | G-DWARF STARS | SOLAR NEIGHBORHOOD | ASTRONOMY & ASTROPHYSICS | STELLAR POPULATIONS | METALLICITY GRADIENT | ELEMENTAL ABUNDANCE | ATMOSPHERIC PARAMETERS | SPECTROSCOPIC SURVEY | Substructures | Algorithms | Planes | Disks | Evolution | Mathematical models | Iron | Chemical evolution | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
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11. Full Text Chemistry in disks: VIII. the CS molecule as an analytic tracer of turbulence in disks
by Guilloteau, S and Dutrey, A and Wakelam, V and Hersant, F and Semenov, D and Chapillon, E and Henning, T and Piétu, V
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 548, p. A70
Context. Turbulence is thought to be a key driver of the evolution of protoplanetary disks, regulating the mass accretion process, the transport of angular... 
Circumstellar matter | Radio lines: planetary systems | Protoplanetary disks | Radio lines: stars | radio lines: planetary systems | MAGNETOHYDRODYNAMIC SIMULATIONS | CHEMICAL EVOLUTION | PROTOPLANETARY ACCRETION DISKS | circumstellar matter | T TAURI DISKS | COLD CO | ASTRONOMY & ASTROPHYSICS | DM-TAU | GAS | CONSTRAINTS | CIRCUMSTELLAR DISKS | protoplanetary disks | FLOWS | radio lines: stars | Physics - Astrophysics of Galaxies | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics
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12. Full Text MAGNETO-THERMAL DISK WINDS from PROTOPLANETARY DISKS
by Bai, Xue-Ning and Ye, Jiani and Goodman, Jeremy and Yuan, Feng
Astrophysical Journal, ISSN 0004-637X, 02/2016, Volume 818, Issue 2, p. 152
The global evolution and dispersal of protoplanetary disks (PPDs) are governed by disk angular-momentum transport and mass-loss processes. Recent numerical... 
protoplanetary disks | methods: numerical | accretion, accretion disks | magnetohydrodynamics (MHD) | MAGNETOROTATIONAL-INSTABILITY | YOUNG STELLAR OBJECTS | ACTIVE GALACTIC NUCLEI | ASTRONOMY & ASTROPHYSICS | ACCRETION-EJECTION STRUCTURES | X-RAY IONIZATION | PLANETESIMAL FORMATION | CIRCUMSTELLAR DISKS | MAGNETICALLY-DRIVEN JETS | T-TAURI STARS | WEAKLY MAGNETIZED DISKS | Stellar winds | Protoplanets | Planet formation | Heating | Planetary evolution | Disks | Magnetic fields | Transport
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13. Full Text Chemistry in disks: VI. CN and HCN in protoplanetary disks
by Chapillon, E and Guilloteau, S and Dutrey, A and Piétu, V and Guélin, M
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 537, p. A60
Context. The chemistry of protoplanetary disks is thought to be dominated by two major processes: photodissociation near the disk surface and depletion on dust... 
protoplanetary disks | astrochemistry | radio lines: stars | circumstellar matter | MOLECULAR CONTENT | INTERSTELLAR CLOUDS | COLD CO | ASTRONOMY & ASTROPHYSICS | LKCA-15 | DM-TAU | X-RAY | GAS | CIRCUMSTELLAR DISKS | T-TAURI STARS | LY-ALPHA RADIATION | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics
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