55 citations · 330 across the 10 of their papers we have counts for
9 papers
PDRs4All XIX. The 6 to 9 m region as a probe of PAH charge and size in the Orion Bar
Baria Khan, Samuel A. Daza Rodriguez, Els Peeters +24
Infrared emission from polycyclic aromatic hydrocarbons (PAHs) play a major role in determining the charge balance of their host environments that include photo-dissociation region…
SOFIA Far-infrared [O III] and [O I] Observations of Dense CO-knots in the Supernova Remnant Cassiopeia A: Multi-phase Ejecta
Jeonghee Rho, Sofia Wallstrom, Sebastien Muller +5
Dense, fast-moving ejecta knots in supernova remnants are prime sites for molecule and dust formation. We present SOFIA far-IR spectrometer FIFI-LS observations of CO-rich knots in…
The Orion HII Region and the Orion Bar in the Mid-Infrared
F. Salgado, O. Berné, J. D. Adams +2
We present mid-infrared photometry of the Orion Bar obtained with FORCAST aboard SOFIA at 6.4, 6.6, 7.7, 19.7, 31.5 and 37.1 \um. By complementing this observations with archival F…
High spatial resolution imaging of SO and H2CO in AB Auriga: the first SO image in a transitional disk
S. Pacheco-Vázquez, A. Fuente, C. Baruteau +6
Transitional disks are structures of dust and gas around young stars with large inner cavities in which planet formation may occur. Lopsided dust distributions are observed in the…
C in Photodissociation Regions
Pablo Castellanos, Olivier Berné, Yaron Sheffer +2
Recent studies have confirmed the presence of buckminsterfullerene (C) in different interstellar and circumstellar environments. However, several aspects regarding C…
Radiation-pressure-driven dust waves inside bursting interstellar bubbles
B. B. Ochsendorf, S. Verdolini, N. L. J. Cox +3
Massive stars drive the evolution of the interstellar medium through their radiative and mechanical energy input. After their birth, they form bubbles of hot gas surrounded by a de…
Blowing in the wind: The dust wave surrounding Ori AB
B. B. Ochsendorf, N. L. J. Cox, S. Krijt +5
Observations with the Spitzer Space Telescope and the WISE satellite have revealed a prominent arc-like structure at 50" ( pc) from the O9.5V/B0.5V system Ori AB. We…
PAH emission in the proplyd HST10: what is the mechanism behind photoevaporation?
Silvia Vicente, Olivier Berne, Alexander G. G. M. Tielens +4
Proplyds are photodissociation region (PDR)-like cometary cocoons around young stars which are thought to originate through photo-evaporation of the central protoplanetary disk by…
First science results from SOFIA/FORCAST: The mid-infrared view of the compact HII region W3A
F. Salgado, O. Berne, J. D. Adams +11
The massive star forming region W3 was observed with the faint object infrared camera for the SOFIA telescope (FORCAST) as part of the Short Science program. The 6.4, 6.6, 7.7, 19.…