The Physical Nature of the Lyman Limit Systems
Jason X. Prochaska
Abstract
We analyze Keck HIRES observations of a Lyman limit system at z=2.652 toward Q2231-00. These observations afford the most comprehensive study of the physical properties of a LL system to date. By comparing the ionic column densities for Fe+, Fe++, Si+, and Si3+ against calculations derived from the CLOUDY software package, we have strictly constrained the ionization state of this system. This has enabled us to calculate accurate abundances of a Lyman limit system for the first time at z > 2, e.g., [Fe/H] = -0.5 0.1. We also derive a total hydrogen column density, log N(H) = 20.73 0.2, which is comparable to values observed for the damped lya systems. The system is special for exhibiting CII* 1335 absorption, allowing an estimate of the electron density, ne = 6.5 1.3 x 10-2 cm-3. Coupling this measurement with our knowledge of the ionization state, we derive the following physical properties: (1) hydrogen volume density, nH = 5.9 1.2 x 10-2 cm-3, (2) path length, l = 3 1.6 kpc, and (3) ionizing intensity, log J912 = -20.22 0.21. We point out that a number of the physical properties (e.g. [Fe/H], N(H), nH) resemble those observed for the damped lya systems, which suggests this system may be the photoionized analog of a damped system. The techniques introduced in this Letter should be applicable to a number of Lyman limit systems and therefore enable a survey of their chemical abundances and other physical properties.
Create a lesson
Related papers
On binary pulsars and the force of gravity
Davor Palle
Tidal torques. A critical review of some techniques
Michael Efroimsky, James G. Williams
Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
Rodrigo Fernández, Christopher Thompson
Asymptotically FRW black holes
J. T. Firouzjaee, Reza Mansouri
Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole Merger
Sean M. O'Neill, M. Coleman Miller, Tamara Bogdanovic et al.
A Gamma-Ray Burst/Pulsar for Cosmic-Ray Positrons with a Dark Matter-like Spectrum
Kunihito Ioka