activity
20082026
most citedThe physical and chemical structure of Sagittarius B2, I. Three-dimensional thermal dust and free-free continuum modeling on 100 au to 45 pc scales

154 citations · 870 across the 52 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2020★ 12 cited

Star Cluster Formation in Orion A

Wanggi Lim, Fumitaka Nakamura, Benjamin Wu +9

We introduce new analysis methods for studying the star cluster formation processes in Orion A, especially examining the scenario of a cloud-cloud collision. We utilize the CARMA-N…

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★ 69 cited

Accelerating infall and rotational spin-up in the hot molecular core G31.41+0.31

M. T. Beltrán, R. Cesaroni, V. M. Rivilla +20

As part of our effort to search for circumstellar disks around high-mass stellar objects, we observed the well-known core G31.41+0.31 with ALMA at 1.4 mm with an angular resolution…

astro-ph.SR2017★ 44 cited

Chemical Segregation in Hot Cores With Disk Candidates: An investigation with ALMA

V. Allen, F. F. S. van der Tak, Á. Sánchez-Monge +2

In the study of high-mass star formation, hot cores are empirically defined stages where chemically rich emission is detected toward a massive YSO. It is unknown whether the physic…

astro-ph.SR2015★ 8 cited

Next Generation Very Large Array Memo No. 6, Science Working Group 1: The Cradle of Life

Andrea Isella, Charles L. H. Hull, Arielle Moullet +33

This paper discusses compelling science cases for a future long-baseline interferometer operating at millimeter and centimeter wavelengths, like the proposed Next Generation Vary L…