activity
19982022
most citedDiagnostics of AGN-driven Molecular Outflows in ULIRGs from Herschel-PACS Observations of OH at 119um

167 citations · 1.8k across the 46 of their papers we have counts for

collaborators

46 papers

astro-ph.HE2022★ 18 cited

Multi-wavelength Variability of Sagittarius A* in July 2019

H. Boyce, D. Haggard, G. Witzel +14

We report timing analysis of near-infrared (NIR), X-ray, and sub-millimeter (submm) data during a three-day coordinated campaign observing Sagittarius A*. Data were collected at 4.…

astro-ph.HE2021★ 64 cited

Constraining particle acceleration in Sgr A* with simultaneous GRAVITY, Spitzer, NuSTAR and Chandra observations

R. Abuter, A. Amorim, M. Bauböck +81

We report the time-resolved spectral analysis of a bright near-infrared and moderate X-ray flare of Sgr A*. We obtained light curves in the -, -, and -bands in the mid- an…

astro-ph.SR2020★ 2 cited

COBRaS: The e-MERLIN 21 cm Legacy survey of Cygnus OB2

J. C. Morford, D. M. Fenech, R. K. Prinja +12

The role of massive stars is central to an understanding of galactic ecology. It is important to establish the details of how massive stars provide radiative, chemical, and mechani…

astro-ph.SR2017★ 3 cited

MWC349A and B Are Not Gravitationally Bound: New Evidence

P. M. Drew, V. Strelnitski, H. A. Smith +3

The age and evolutionary status of MWC349A, the unique emission line star with maser and laser radiation in hydrogen recombination lines, remain unknown because the spectrum of the…

astro-ph.GA2016★ 164 cited

Molecular outflows in local ULIRGs: energetics from multi-transition OH analysis

E. González-Alfonso, J. Fischer, H. W. W. Spoon +11

We report on the energetics of molecular outflows in 14 local Ultraluminous Infrared Galaxies (ULIRGs) that show unambiguous outflow signatures (P-Cygni profiles or high-velocity a…

astro-ph.SR2015

SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment

J. D. Adams, T. L. Herter, J. L. Hora +22

We present mid-IR (19 - 37 microns) imaging observations of S106 from SOFIA/FORCAST, complemented with IR observations from Spitzer/IRAC (3.6 - 8.0 microns), IRTF/MIRLIN (11.3 and…