595 citations · 3.3k across the 60 of their papers we have counts for
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Changes Of Dust Opacity With Density in the Orion A Molecular Cloud
Arabindo Roy, Peter G. Martin, Danae Polychroni +12
We have studied the opacity of dust grains at submillimeter wavelengths by estimating the optical depth from imaging at 160, 250, 350, and 500 um from the Herschel Gould Belt Surve…
Herschel view of the Taurus B211/3 filament and striations: Evidence of filamentary growth?
P. Palmeirim, Ph. André, J. Kirk +23
We present first results from the Herschel Gould Belt survey for the B211/L1495 region in the Taurus molecular cloud. Thanks to their high sensitivity and dynamic range, the Hersch…
Estimating distance, pressure, and dust opacity using submillimeter observations of self-gravitating filaments
Joerg Fischera, Peter G. Martin
We present a detailed study of the surface brightness profiles of dense filaments in IC 5146 using recent Herschel observations done with SPIRE. We describe the profile through an…
Physical properties of interstellar filaments
Joerg Fischera, Peter G. Martin
We analyze the physical parameters of interstellar filaments that we describe by an idealized model of isothermal self-gravitating infinite cylinder in pressure equilibrium with th…
Evolution of dust in the Orion Bar with Herschel: I. Radiative transfer modelling
Heddy Arab, Alain Abergel, Emilie Habart +5
Interstellar dust is a key element in our understanding of the interstellar medium and star formation. The manner in which dust populations evolve with the excitation and the physi…