activity
20172020
most citedThe Radial Distribution of Dust Particles in the HL Tau Disk from ALMA and VLA Observations

175 citations · 464 across the 8 of their papers we have counts for

collaborators

11 papers

astro-ph.SR202011 cited

Pebbles in an Embedded Protostellar Disk: The Case of CB26

Chuan-Peng Zhang, Ralf Launhardt, Yao Liu +2

Planetary cores are thought to form in proto-planetary disks via the growth of dusty solid material. However, it is unclear how early this process begins. We study the physical str…

astro-ph.EP202039 cited

Dual-Wavelength ALMA Observations of Dust Rings in Protoplanetary Disks

Feng Long, Paola Pinilla, Gregory J. Herczeg +13

We present new Atacama Large Millimeter/submillimeter Array (ALMA) observations for three protoplanetary disks in Taurus at 2.9\,mm and comparisons with previous 1.3\,mm data both…

astro-ph.IM20201 cited

Bringing high spatial resolution to the Far-infrared -- A giant leap for astrophysics

Hendrik Linz, Henrik Beuther, Maryvonne Gerin +11

The far-infrared (FIR) regime is one of the few wavelength ranges where no astronomical data with sub-arcsecond spatial resolution exist. Neither of the medium-term satellite proje…

astro-ph.EP2019175 cited

The Radial Distribution of Dust Particles in the HL Tau Disk from ALMA and VLA Observations

Carlos Carrasco-González, Anibal Sierra, Mario Flock +13

Understanding planet formation requires to discern how dust grows in protoplanetary disks. An important parameter to measure in disks is the maximum dust grain size present. This i…

astro-ph.SR2019

Compact Disks in a High Resolution ALMA Survey of Dust Structures in the Taurus Molecular Cloud

Feng Long, Gregory J. Herczeg, Daniel Harsono +24

We present a high-resolution (, au, mean sensitivity of Jy~beam at 225 GHz) snapshot survey of 32 protoplanetary disks around young stars with spe…

astro-ph.SR2019152 cited

The newborn planet population emerging from ring-like structures in discs

G. Lodato, G. Dipierro, E. Ragusa +23

ALMA has observed a plethora of ring-like structures in planet forming discs at distances of 10-100 au from their host star. Although several mechanisms have been invoked to explai…