We explain the axisymmetric gaps seen in recent long-baseline observations of the HL Tau
protoplanetary disc with the Atacama Large Millimetre/Submillimetre Array (ALMA) as being …

The detection of Earth-sized exoplanets around low-mass stars–in stars such as Proxima
Centauri and TRAPPIST-1–provide an exceptional chance to improve our understanding of …

Characterizing the physical properties of dust grains in a protoplanetary disk is critical to
comprehending the planet formation process. Our study presents Atacama Large Millimeter …

We present 3D 'zoom-in'simulations of the formation of two molecular clouds out of the
galactic interstellar medium. We model the clouds–identified from the SILCC simulations …

Abstract We present Atacama Large Millimeter/sub-millimeter Array (ALMA) Cycle 2
observations of the 1.3-mm dust continuum emission of the protoplanetary disc surrounding …

Episodic accretion has been used to explain the wide range of protostellar luminosities, but
its origin and influence on the star-forming process are not yet fully understood. We present …

We have investigated the protostellar disk around a Class 0/I protostar, L1527 IRS, using
multiwavelength observations of the dust continuum emission at λ= 0.87, 2.1, 3.3, and 6.8 …

The disk of HD 163296 shows ring and gap substructures in observations with the Atacama
Large Millimeter/submillimeter Array. In addition, this is the only disk where the rings and …

We present a model of the early chemical composition and elemental abundances of
planetary atmospheres based on the cumulative gaseous chemical species that are …

The accurate measurement of temperature in protoplanetary disks is critical to
understanding many key features of disk evolution and planet formation, from disk chemistry …