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Astronomy and astrophysics (Berlin), ISSN 0004-6361, 09/2018, Volume 617, p. A28
Context. Several sulfur-bearing molecules are observed in the interstellar medium and in comets, in strong contrast to protoplanetary disks where only CS, H2CS, and SO have been detected so far. Aims... 
Circumstellar matter | Astrochemistry | Radio lines: planetary systems | Protoplanetary disks | Radio lines: stars | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Solar and Stellar Astrophysics | Earth and Planetary Astrophysics | Astrophysics | Physics
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2012, Volume 537, p. A60
Journal Article
Annual review of astronomy and astrophysics, ISSN 0066-4146, 9/2011, Volume 49, Issue 1, pp. 195 - 236
Protoplanetary disks are quasi-steady structures whose evolution and dispersal determine the environment for planet formation... 
pre-main-sequence stars | accretion | protoplanetary disks | Protoplanetary disks | Pre-main-sequence stars | Accretion | Astrophysics | Research | Planetary rings | Properties | Observations | Dynamics | Magnetization | Planet formation | Ionization | Planetary evolution | Stars | Disks | Planetary probes
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2015, Volume 574, p. A68
Aims. Recent observations by the Atacama Large Millimeter/submillimeter Array (ALMA) of disks around young stars revealed distinct asymmetries in the dust continuum emission... 
Submillimeter: Planetary systems | Turbulence | Accretion | Protoplanetary disks | Magnetohydrodynamics (MHD) | Instabilities | Accretion disks | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Magnetohydrodynamics | Turbulent flow | Computer simulation | Protoplanets | Planet formation | Radio telescopes | MHD | Physics | Astrophysics
Journal Article