The Physics of the Far-infrared-Radio Correlation. II. Synchrotron Emission as a Star Formation Tracer in High-redshift Galaxies

We construct one-zone steady-state models of cosmic ray (CR) injection, cooling, and escape over the entire dynamic range of the FIR-radio correlation (FRC), from normal galaxies to starbursts, over the redshift interval 0 {

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Bibliographic Details
Published in:The Astrophysical journal 2010-07, Vol.717 (1), p.196-208
Main Authors: Lacki, Brian C, Thompson, Todd A
Format: Article
Language:English
Subjects:
ANTILEPTONS
ANTIMATTER
ANTIPARTICLES
Astronomy
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BREMSSTRAHLUNG
BRIGHTNESS
COSMIC RADIATION
Earth, ocean, space
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
EMISSION
ENERGY DENSITY
EVOLUTION
Exact sciences and technology
FERMIONS
GALACTIC EVOLUTION
GALAXIES
IONIZATION
IONIZING RADIATIONS
LEPTONS
LUMINOSITY
MAGNETIC FIELDS
MATTER
MICROWAVE RADIATION
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
POSITRONS
RADIATIONS
RED SHIFT
RELICT RADIATION
STARS
STEADY-STATE CONDITIONS
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Description
Summary:We construct one-zone steady-state models of cosmic ray (CR) injection, cooling, and escape over the entire dynamic range of the FIR-radio correlation (FRC), from normal galaxies to starbursts, over the redshift interval 0 {
ISSN:0004-637X
1538-4357
DOI:10.1088/0004-637X/717/1/196