activity
20172019
most citedSubstructures in the Keplerian disc around the O-type (proto)star G17.64+0.16

79 citations · 125 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2019

Exploring the formation pathways of formamide near young O-type stars

Veronica Allen, Floris F. S. van der Tak, Ana López-Sepulcre +4

Context. As a building block for amino acids, formamide (NHCHO) is an important molecule in astrobiology and astrochemistry, but its formation path in the interstellar medium i…

astro-ph.SR201979 cited

Substructures in the Keplerian disc around the O-type (proto)star G17.64+0.16

L. T. Maud, R. Cesaroni, M. S. N. Kumar +20

We present the highest angular resolution (20x15mas - 44x33au) Atacama Large Millimeter/sub-millimeter Array (ALMA) observations currently possible of the proto-O-star G17.64+0.16…

astro-ph.EP20192 cited

Impacts of Quantum Chemistry Calculations on Exoplanetary Science, Planetary Astronomy, and Astrophysics

Der-you Kao, Marko Gacesa, Renata M. Wentzcovitch +26

Several of NASA missions (TESS, JWST, WFIRST, etc.) and mission concepts (LUVOIR, HabEx, and OST) emphasize the exploration and characterization of exoplanets, and the study of the…

astro-ph.SR2018

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.GA2018

Complex cyanides as chemical clocks in hot cores

V. Allen, F. F. S. van der Tak, C. Walsh

In the high-mass star-forming region G35.20-0.74N, small scale (about 800 AU) chemical segregation has been observed in which complex organic molecules containing the CN group are…

astro-ph.SR2018

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…