activity
20152022
most citedDust masses of young disks: constraining the initial solid reservoir for planet formation

204 citations · 1.9k across the 38 of their papers we have counts for

collaborators

51 papers

astro-ph.EP202212 cited

ALMA constraints on assembly of Core Accretion planets

Sergei Nayakshin, Vardan Elbakyan, Giovanni Rosotti

Resolved dust continuum and CO line ALMA imaging, and in some cases detection of H emission, hint that young massive planets are abundant at wide separations in protoplanetary d…

astro-ph.EP202270 cited

Gas Disk Sizes from CO Line Observations: A Test of Angular Momentum Evolution

Feng Long, Sean M. Andrews, Giovanni Rosotti +7

The size of a disk encodes important information about its evolution. Combining new Submillimeter Array (SMA) observations with archival Atacama Large Millimeter Array (ALMA) data,…

astro-ph.EP202214 cited

Characteristics of small protoplanetary disc warps in kinematic observations

Alison K. Young, Richard Alexander, Giovanni Rosotti +1

Many circumstellar discs appear to have misaligned central regions that give rise to shadows seen in scattered light observations. Small warps ( misalignment) are probab…

astro-ph.SR202220 cited

Stellar multiplicity affects the correlation between proto-planetary disc masses and accretion rates: binaries explain high-accretors in Upper Sco

Francesco Zagaria, Cathie J. Clarke, Giovanni P. Rosotti +1

In recent years a correlation between mass accretion rates onto new-born stars and their proto-planetary disc masses was detected in nearby young star-forming regions. Although suc…

astro-ph.EP202240 cited

A large population study of protoplanetary disks: Explaining the millimeter size-luminosity relation with or without sub-structure

Apostolos Zormpas, Tilman Birnstiel, Giovanni P. Rosotti +1

Recent sub-arcsecond resolution surveys of the dust continuum emission from nearby protoplanetary disks showed a strong correlation between the sizes and luminosities of the disks.…

astro-ph.EP202157 cited

On the secular evolution of the ratio between gas and dust radii in protoplanetary discs

Claudia Toci, Giovanni Rosotti, Giuseppe Lodato +2

A key problem in protoplanetary disc evolution is understanding the efficiency of dust radial drift. This process makes the observed dust disc sizes shrink on relatively short time…