The Sunyaev-Zel'dovich effect due to hyper-starburst galaxy winds
arXiv:1005.4234 · doi:10.1111/j.1365-2966.2010.17953.x
Abstract
We construct a simple, spherical blastwave model to estimate the pressure structure of the intergalactic medium surrounding hyper-starburst galaxies, and argue that the effects of interaction with star-forming galaxy winds may be approximated at early times by an adiabatically expanding, self-similar `bubble' as described by Weaver et al. (1977) and Ostriker & McKee (1988). This model is used to make observational predictions for the thermal Sunyaev-Zel'dovich effect in the shocked bubble plasma. Radiative cooling losses are explored, and it is found that bremsstrahlung will limit the epoch of adiabatic expansion to -- years: comparable to total hyper-starburst lifetimes. Prospects for making a first Sunyaev-Zel'dovich detection of galaxy wind bubbles using the Atacama Large Millimeter Array are examined for a number of active hyper-starburst sources in the literature.
6 pages, 2 figures, 1 table. Version accepted for publication in MNRAS
References in corpus (25)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Ubiquitous outflows in DEEP2 spectra of star-forming galaxies at z=1.4
- A Kiloparsec-Scale Hyper-Starburst in a Quasar Host Less than 1 Gigayear after the Big Bang
- The Persistence of Cool Galactic Winds in High Stellar Mass Galaxies Between z~1.4 and ~1
- Thermal Emission from Warm Dust in the Most Distant Quasars
- Spectroscopic Confirmation Of An Extreme Starburst At Redshift 4.547
- A submillimetre galaxy at z=4.76 in the LABOCA survey of the Extended Chandra Deep Field South
- Molecular Gas in a Submillimeter Galaxy at z=4.5: Evidence for a Major Merger at 1 Billion Years after the Big Bang
- Imaging Atomic and Highly Excited Molecular Gas in a z=6.42 Quasar Host Galaxy: Copious Fuel for an Eddington-Limited Starburst at the End of Cosmic Reionization
- Detection of Two Massive CO Systems in 4C 41.17 at z = 3.8
- Confirming a Population of Hot-Dust Dominated, Star Forming Ultraluminous Galaxies at High-Redshift
- Molecular gas in QSO host galaxies at z>5
- Multi-frequency imaging of the galaxy cluster Abell 2163 using the Sunyaev-Zel'dovich Effect
- The Sunyaev-Zel'dovich effects from a cosmological hydrodynamical simulation: large-scale properties and correlation with the soft X-ray signal
- Neutral Gas Outflows and Inflows in Infrared-Faint Seyfert Galaxies
- Non-parametric modeling of the intra-cluster gas using APEX-SZ bolometer imaging data
- Constrained semi-analytical models of Galactic outflows
- Measuring AGN Feedback with the Sunyaev-Zel'dovich Effect
- Millimetre observations of a sample of high-redshift obscured quasars
- Simulations of the Sunyaev-Zeldovich Effect from Quasars
- The Sunyaev-Zeldovich Effect from Quasar Feedback
- CMB Anisotropies from Outflows in Lyman Break Galaxies
- Radio and X-ray properties of submillimeter galaxies in the A2125 field
- Search for the Sunyaev-Zel'dovich Effect in a Giant Radio Galaxy B1358+305
- Sunyaev-Zel'dovich Effect Observations of the Bullet Cluster (1E 0657-56) with APEX-SZ