606 citations · 12.5k across the 161 of their papers we have counts for
164 papers
Radio multiwavelength analysis of the compact disk CX Tau: Presence of strong free-free variability or anomalous microwave emission
Pietro Curone, Leonardo Testi, Enrique Macias +8
Protoplanetary disks emit radiation across a broad range of wavelengths, requiring a multiwavelength approach to fully understand their physical mechanisms and how they form planet…
Testing protoplanetary disc evolution with CO fluxes. A proof of concept in Lupus and Upper Sco
Francesco Zagaria, Stefano Facchini, Anna Miotello +3
The Atacama Large Millimeter/submillimeter Array (ALMA) revolutionised our understanding of protoplanetary discs. However, the available data have not given conclusive answers yet…
Accretion of sub-stellar companions as the origin of chemical abundance inhomogeneities in globular clusters
Andrew J. Winter, Cathie J. Clarke
Globular clusters exhibit abundance variations, defining `multiple populations', which have prompted a protracted search for their origin. Properties requiring explanation include:…
Dust dynamics in planet-forming discs in binary systems
Francesco Zagaria, Giovanni P. Rosotti, Richard D. Alexander +1
In multiple stellar systems interactions among the companion stars and their discs affect planet formation. In the circumstellar case tidal truncation makes protoplanetary discs sm…
Forming short period sub-stellar companions in 47 Tucanae -- II. Analytic expressions for the orbital evolution of planets in dense environments
Andrew J. Winter, Cathie J. Clarke, Giovanni Rosotti +1
Short period, massive planets, known as hot Jupiters (HJs), have been discovered around percent of local field stars. The inward migration necessary to produce HJs may be…
Super-resolution trends in the ALMA Taurus survey: Structured inner discs and compact discs
Jeff Jennings, Marco Tazzari, Cathie J. Clarke +2
The 1.33 mm survey of protoplanetary discs in the Taurus molecular cloud found annular gaps and rings to be common in extended sources (>~55 au), when their 1D visibility distribut…