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The Astrophysics of Star Formation Across Cosmic Time at 10 GHz with the Square Kilometre Array
Eric J. Murphy, Mark T. Sargent, Rob J. Beswick +12
In this chapter, we highlight a number of science investigations that are enabled by the inclusion of Band~5 ( GHz) for SKA1-MID science operations, while focusing on the…
Dust continuum emission as a tracer of gas mass in galaxies
Brent A. Groves, Eva Schinnerer, Adam Leroy +8
We use a sample of 36 galaxies from the KINGFISH (Herschel IR), HERACLES (IRAM CO), and THINGS (VLA HI) surveys to study empirical relations between Herschel infrared (IR) luminosi…
The Herschel Virgo Cluster Survey. XVII. SPIRE point-source catalogs and number counts
Ciro Pappalardo, George J. Bendo, Simone Bianchi +19
We present three independent catalogs of point-sources extracted from SPIRE images at 250, 350, and 500 micron as a part of the Herschel Virgo Cluster Survey (HeViCS). The source p…
Cool dust heating and temperature mixing in nearby star-forming galaxies
L. K. Hunt, B. T. Draine, S. Bianchi +20
Physical conditions of the interstellar medium in galaxies are closely linked to the ambient radiation field and the heating of dust grains. In order to characterize dust propertie…
Are LGRBs biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of LGRBs. I: Stellar mass at z<1
S. D. Vergani, R. Salvaterra, J. Japelj +20
LGRBs are associated with massive stars and are therefore linked to star formation. The conditions necessary to produce LGRBs can affect the relation between the LGRB rate and star…
A quiescent galaxy at the position of the long GRB 050219A
A. Rossi, S. Piranomonte, S. Savaglio +25
Long-duration gamma-ray bursts (LGRBs) are produced by the collapse of very massive stars. Due to the short lifetime of their progenitors, LGRBs pinpoint star-forming galaxies. We…