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20072026
most citedGaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region

530 citations · 5.5k across the 90 of their papers we have counts for

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Showing 2018Show all

12 papers · 1 filter

astro-ph.EP2018★ 72 cited

The Ring Structure in the MWC 480 Disk Revealed by ALMA

Yao Liu, Giovanni Dipierro, Enrico Ragusa +20

Gap-like structures in protoplanetary disks are likely related to planet formation processes. In this paper, we present and analyze high resolution (0.17*0.11 arcsec) 1.3 mm ALMA c…

astro-ph.SR2018★ 530 cited

Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region

Feng Long, Paola Pinilla, Gregory J. Herczeg +23

Rings are the most frequently revealed substructure in ALMA dust observations of protoplanetary disks, but their origin is still hotly debated. In this paper, we identify dust subs…

astro-ph.SR2018★ 64 cited

Chasing discs around O-type (proto)stars - ALMA evidence for an SiO disc and disc wind from G17.64+0.16

L. T. Maud, R. Cesaroni, M. S. N. Kumar +28

We present high angular resolution 0.2 arcsec continuum and molecular emission line Atacama Large Millimeter/sub-millimeter Array (ALMA) observations of G17.64+0.16 in Band 6 (220G…

astro-ph.SR2018★ 92 cited

Methanol and its relation to the water snowline in the disk around the young outbursting star V883 Ori

Merel L. R. van 't Hoff, John J. Tobin, Leon Trapman +5

We report the detection of methanol in the disk around the young outbursting star V883 Ori with the Atacama Large Millimeter/submillimeter Array (ALMA). Four transitions are observ…

astro-ph.SR2018★ 16 cited

Revised SED of the triple protostellar system VLA 1623-2417

Nadia M. Murillo, Daniel Harsono, Melissa McClure +2

VLA 16232417 is a triple protostellar system deeply embedded in Ophiuchus A. Sources A and B have a separation of 1.1", making their study difficult beyond the submillimeter reg…

astro-ph.SR2018★ 100 cited

Evidence for the start of planet formation in a young circumstellar disk

Daniel Harsono, Per Bjerkeli, Matthijs H. D. van der Wiel +4

The growth of dust grains in protoplanetary disks is a necessary first step towards planet formation. This growth has been inferred via observations of thermal dust emission toward…