NOAO >   Observing Info >   Approved Programs >   2014A-0266

Small NOAO Logo

Proposal Information for 2014A-0266


PI: Michele Fumagalli, Carnegie Institution for Science, mfumagalli@obs.carnegiescience.edu
Address: The Observatories, 813 Santa Barbara St., Pasadena, CA 91101, USA

CoI: Joseph Hennawi, Max Planck Institute for Astronomy
CoI: Adam Myers, University of Wyoming

Title: Resolving the small-scale structure of the circumgalactic medium at z~3

Abstract: Modern cosmological simulations predict that in the distant Universe the bulk of cold gas is never shock-heated, but rather cold mode accretion occurs along dense filaments of the cosmic web. Although these ``cold streams'' are postulated to give rise to Lyman limit system (LLS) absorption arising from the circumgalactic medium (CGM) of galaxies, the connection between LLSs and galaxies has been extremely difficult to establish, because of the dearth of galaxy-quasar pairs at small separations. Here we adopt a novel approach, and propose to measure the small-scale structure and clustering of LLSs. By targeting quasar pairs with projected separations 1-250 \rm kpc at z\ge3, we will measure the incidence of correlated absorption at the Lyman limit. The shape of the resulting correlation function directly tests the link between LLSs and galaxies, and simultaneously measures the covering factor of optically-thick hydrogen in the CGM of z~ 3 galaxies. These observations will also yield a large sample of LLS-pairs, constraining the degree of small-scale metal mixing and the amount of velocity shear inside galactic halos.


National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360



NOAO >   Observing Info >   Approved Programs >   2014A-0266

noaoprop-help@noao.edu

Small NOAO Logo