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Astrophysical journal. Letters, ISSN 2041-8213, 2019, Volume 885, Issue 1, p. L27
Journal Article
Science (American Association for the Advancement of Science), ISSN 1095-9203, 2016, Volume 353, Issue 6307, pp. 1519 - 1521
Gravitational forces are expected to excite spiral density waves in protoplanetary disks, disks of gas and dust orbiting young stars. However, previous... 
EVOLUTION | SIGNATURES | IMAGES | MULTIDISCIPLINARY SCIENCES | MASS | ARMS | ACCRETION | OPHIUCHUS | GRAVITATING CIRCUMSTELLAR DISCS | EMISSION | Analysis | Planetary nebulae | Gravity | Protoplanetary disks | Star & galaxy formation | Gravitational waves | Protostars | Spirals | Protoplanets | Planet formation | Stars | Planetary probes | Arrays | Accretion disks | Density
Journal Article
The Astronomical journal, ISSN 1538-3881, 2017, Volume 153, Issue 5, p. 240
The σ  Orionis cluster is important for studying protoplanetary disk evolution, as its intermediate age (∼3–5 Myr) is comparable to the median disk lifetime.... 
stars: pre-main sequence | accretion accretion disks | protoplanetary disks | stars: protostars | planets and satellites: formation | circumstellar matter | PLANETS | CARBON 13 | CARBON 12 | PROTOPLANETS | CARBON 18 | COMPARATIVE EVALUATIONS | ACCRETION DISKS | CARBON MONOXIDE | LIFETIME | STAR CLUSTERS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MASS | PROTOSTARS | STARS | DETECTION | SATELLITES | EMISSION | COSMIC DUST
Journal Article
Icarus (New York, N.Y. 1962), ISSN 0019-1035, 01/2020, Volume 335, p. 113380
Most major planetary bodies in the Solar System rotate in the same direction as their orbital motion: their spin is prograde. Theoretical studies to explain... 
ROTATION | ANGULAR-MOMENTUM | ORIGIN | PARTICLES | STATISTICS | ASTRONOMY & ASTROPHYSICS | MASS | GROWTH | GRADUAL ACCUMULATION | PROTOPLANETS | TERRESTRIAL PLANETS
Journal Article
Astrophysical journal. Letters, ISSN 2041-8205, 06/2018, Volume 860, Issue 1, p. L12
Journal Article
The Astrophysical journal, ISSN 0004-637X, 2017, Volume 851, Issue 2, p. 83
We present a high angular resolution (\(\sim 0\buildrel{\prime\prime}\over{.} 2\)), high-sensitivity (\(\sigma \sim 0.2\) mJy) survey of the 870 μm continuum... 
stars: formation | stars: pre-main sequence | protoplanetary disks | Fluctuations | Angular resolution | Molecular clouds | Flux | Protoplanetary disk | Probability distribution | Infrared signatures | Accretion disks | Surveys | Wavelengths | Protoplanets | Northern Hemisphere | Planet formation | Binary stars | Millimeter waves | Continuum radiation | Pre-main sequence stars
Journal Article