One of the most active fields of research in accretion disk theory is understanding the mechanisms that transport angular momentum outward. Two instabilities are thought to be responsible for it in massive, magnetized disks: the magnetorotational instability (MRI) caused by the presence of a weak magnetic field, and gravitational instabilities.This PhD
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Earth-mass planets with He atmospheres in the habitable zone of Sun-like stars. [PDF]
Lammer H +6 more
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Interstellar ices as carriers of supernova material to the early solar system. [PDF]
Bizzarro M +12 more
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Chondrule formation by collisions of planetesimals containing volatiles triggered by Jupiter's formation. [PDF]
Sirono SI, Turrini D.
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A precise metallicity and carbon-to-oxygen ratio for a warm giant exoplanet from its panchromatic JWST emission spectrum. [PDF]
Wiser LS +13 more
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The Origins & Reservoirs of Exocomets. [PDF]
Bannister M +13 more
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Fundamentals of Interior Modelling and Challenges in the Interpretation of Observed Rocky Exoplanets. [PDF]
Baumeister P +9 more
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Dust traps in protoplanetary disks efficiently form organic macromolecular matter
Ligterink N +6 more
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Laboratory Investigation of Simultaneous Ultraviolet Photoprocessing and Temperature-Programmed Desorption of Interstellar Ice Analogs. [PDF]
Sarver CC, Walker CE, Widicus Weaver SL.
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