activity
20182020
most citedThe HO Spectrum of the Massive Protostar AFGL 2136 IRS 1 from 2 to 13 m at High Resolution: Probing the Circumstellar Disk

15 citations · 16 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20201 cited

High Resolution Infrared Spectroscopy of Hot Molecular Gas in AFGL 2591 and AFGL 2136: Accretion in the Inner Regions of Disks Around Massive Young Stellar Objects

Andrew G. Barr, Adwin Boogert, Curtis N. DeWitt +8

We have performed a high resolution 4-13 spectral survey of the hot molecular gas associated with the massive protostars AFGL 2591 and AFGL 2136, utilising the Echelon-Cross-E…

astro-ph.SR202015 cited

The HO Spectrum of the Massive Protostar AFGL 2136 IRS 1 from 2 to 13 m at High Resolution: Probing the Circumstellar Disk

Nick Indriolo, D. A. Neufeld, A. G. Barr +6

We have observed the massive protostar AFGL 2136 IRS 1 in multiple wavelength windows in the near-to-mid-infrared at high ( km s) spectral resolution using VLT+CRIRES…

astro-ph.SR2019

Molecular complexity on disk-scales uncovered by ALMA: The chemical composition of the high-mass protostar AFGL 4176

Eva G. Bøgelund, Andrew G. Barr, Vianney Taquet +4

The chemical composition of high-mass protostars reflects the physical evolution associated with different stages of star formation. In this study, the molecular inventory of the f…

astro-ph.SR2018

High-Resolution SOFIA/EXES Spectroscopy of Gas in the Massive Young Stellar Object MonR2 IRS3: Implications for the Sulfur Budget

Ryan Dungee, Adwin Boogert, Curtis N. DeWitt +10

Sulfur has been observed to be severely depleted in dense clouds leading to uncertainty in the molecules that contain it and the chemistry behind their evolution. Here, we aim to s…

astro-ph.GA2018

Infrared Detection of Abundant CS in the Hot Core AFGL 2591 at High Spectral Resolution with SOFIA/EXES

Andrew G. Barr, Adwin Boogert, Curtis N. DeWitt +8

We have performed a 5-8 m spectral line survey of the hot molecular core associated with the massive protostar AFGL 2591, using the Echelon-Cross-Echelle Spectrograph (EXES) on…