155 citations · 370 across the 8 of their papers we have counts for
7 papers · 1 filter
Widespread SiO and CH3OH emission in Filamentary Infrared Dark Clouds
G. Cosentino, I. Jimenez-Serra, J. D. Henshaw +6
Infrared-Dark Clouds (IRDCs) are cold, dense regions of high (optical and infrared) extinction, believed to be the birthplace of high-mass stars and stellar clusters. The physical…
SOLIS II. Carbon-chain growth in the Solar-type protocluster OMC2-FIR4
F. Fontani, C. Ceccarelli, C. Favre +42
The interstellar delivery of carbon atoms locked into molecules might be one of the key ingredients for the emergence of life. Cyanopolyynes are carbon chains delimited at their tw…
Mid-J CO Shock Tracing Observations of Infrared Dark Clouds III: SLED fitting
A. Pon, M. J. Kaufman, D. Johnstone +6
Giant molecular clouds contain supersonic turbulence that can locally heat small fractions of gas to over 100 K. We run shock models for low-velocity, C-type shocks propagating int…
Kompaneets Model Fitting of the Orion-Eridanus Superbubble II: Thinking Outside of Barnard's Loop
Andy Pon, Bram B. Ochsendorf, João Alves +3
The Orion star-forming region is the nearest active high-mass star-forming region and has created a large superbubble, the Orion-Eridanus superbubble. Recent work by Ochsendorf et…
Kompaneets Model Fitting of the Orion-Eridanus Superbubble
Andy Pon, Doug Johnstone, John Bally +1
Winds and supernovae from OB associations create large cavities in the interstellar medium referred to as superbubbles. The Orion molecular clouds are the nearest high mass star-fo…
Mid-J CO observations of Perseus B1-East 5: evidence for turbulent dissipation via low-velocity shocks
Andy Pon, Doug Johnstone, Michael J. Kaufman +2
Giant molecular clouds contain supersonic turbulence and magnetohydrodynamic simulations predict that this turbulence should decay rapidly. Such turbulent dissipation has the poten…