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Triggered/sequential star formation? A multi-phase ISM study around the prominent IRDC G18.93-0.03
J. Tackenberg, H. Beuther, R. Plume +5
G18.93-0.03 is a prominent dust complex within an 0.8deg long filament, with the molecular clump G18.93/m being IR dark from near IR wavelength up to 160mu. Spitzer composite image…
Extended warm and dense gas towards W49A: starburst conditions in our Galaxy?
Z. Nagy, F. F. S. van der Tak, G. A. Fuller +2
The star formation rates in starburst galaxies are orders of magnitude higher than in local star-forming regions, and the origin of this difference is not well understood. We use s…
Star formation towards the Scutum tangent region and the effects of Galactic environment
D. J. Eden, T. J. T. Moore, R. Plume +1
By positional matching to the catalogue of Galactic Ring Survey molecular clouds, we have derived distances to 793 Bolocam Galactic Plane Survey (BGPS) sources out of a possible 80…
Cores in Infra-Red Dark Clouds (IRDCs) seen in the Hi-GAL survey between l = 300° and l = 330°
L. A. Wilcock, D. Ward-Thompson, J. M. Kirk +15
We have used data taken as part of the Herschel infrared Galactic Plane survey (Hi-GAL) to study 3171 infrared-dark cloud (IRDC) candidates that were identified in the mid-infrared…