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Astrophysical Journal, ISSN 0004-637X, 07/2018, Volume 862, Issue 1, p. 45
Journal Article
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622, p. L6
We present a high-resolution numerical study of the phase-space diversity in an isolated Milky Way-type galaxy. Using a single N-body simulation (N approximate... 
Galaxies: evolution | galaxies: kinematics and dynamics | galaxy: kinematics and dynamics | galaxy: disk | Galaxy: disk | INSTABILITY | MODELS | galaxies: evolution | Galaxy: kinematics and dynamics | DISC | VERTICAL STRUCTURE | ASTRONOMY & ASTROPHYSICS | DYNAMICS | BULGES | Spirals
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2009, Volume 397, Issue 3, pp. 1599 - 1606
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2017, Volume 598, p. A66
In this work, two new axisymmetric models for the Galactic mass distribution are presented. Motivated by recent results, these two models include the... 
Galaxy: structure | Galaxy: kinematics and dynamics | Galaxy: disk | STELLAR ORBITS | ROTATION CURVE | SPACE VELOCITIES | LOCAL STANDARD | LIGHT | STAR-FORMATION | FORMATION HISTORY | GALAXY | ASTRONOMY & ASTROPHYSICS | DARK-MATTER | SCALE LENGTH | Physics - Astrophysics of Galaxies | Physics | Astrophysics
Journal Article
The Astrophysical journal, ISSN 0004-637X, 12/2019, Volume 887, Issue 2, p. 148
As the remnants of stars with initial masses less than or similar to 8M(circle dot), white dwarfs contain valuable information on the formation histories of... 
MONTE-CARLO | MASS-DISTRIBUTION | SKY-SURVEY | SOLAR NEIGHBORHOOD | THICK DISC | ASTRONOMY & ASTROPHYSICS | STELLAR HALO | COOLING SEQUENCE | METALLICITY | LUMINOSITY FUNCTION | AGE | White dwarf stars | Galaxies | Milky Way Galaxy | Stellar evolution | Infrared astronomy | Helium | Milky Way | Surveys | Stellar populations | Infrared telescopes | Star formation | Telescopes | Star & galaxy formation | Photometry
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622, p. A86
Globular clusters (GCs), the oldest stellar systems observed in the Milky Way, have long been considered single stellar populations. As such, they provided an... 
Galaxy: evolution | Galaxy: disk | Globular clusters: general | Galaxy: formation | Galaxy: kinematics and dynamics | ABUNDANCE VARIATIONS | PATTERNS | STRENGTHS | ORIGIN | OMEGA-CENTAURI | globular clusters: general | ASTRONOMY & ASTROPHYSICS | MULTIPLE POPULATIONS | STELLAR POPULATIONS | BINARY STAR-CLUSTERS | GIANT BRANCH | DWARF GALAXY
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2018, Volume 863, Issue 2, p. 113
We investigate the nature of the double color-magnitude sequence observed in the Gaia DR2 HR diagram of stars with high transverse velocities. The stars in the... 
Galaxy: halo | Galaxy: evolution | Galaxy: kinematics and dynamics | ASTRONOMY & ASTROPHYSICS | SDSS | METAL-POOR STARS | GALACTIC HALO | KINEMATICS | Organic chemistry | Accretion | Star formation | Galaxies | Galactic disk | Stars | Color | Milky Way Galaxy | Milky Way | Star & galaxy formation | Rotation | Deposition | Physics - Astrophysics of Galaxies | Physics | Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 10/2017, Volume 848, Issue 2, p. 128
Journal Article