Bimodality in Damped Lyman alpha Systems

TL;DR

This paper presents evidence for a bimodal distribution in damped Lyman alpha systems based on cooling rates, revealing two distinct populations with different properties and possible links to galaxy evolution.

Contribution

It identifies a bimodal distribution in DLAs using [C II] cooling rates and explores their properties, star formation modes, and potential connection to galaxy bimodality.

Findings

Two peaks in cooling rate distribution at lc=10^-27.4 and 10^-26.6 ergs s^-1 H^-1.

High cool DLAs have larger metallicity, velocity width, dust-to-gas ratio, and Si II equivalent width.

Bimodality in DLAs may be related to the bimodal properties of nearby galaxies.

Abstract

We report evidence for a bimodality in damped Ly systems (DLAs). Using [C II] 158 mu cooling rates, lc, we find a distribution with peaks at lc=10^-27.4 and 10^-26.6 ergs s^-1 H^-1 separated by a trough at lc^crit ~= lc < 10^-27.0 ergs s^-1 H^-1. We divide the sample into low cool DLAs with lc < lc^crit and high cool DLAs with lc > lc^crit and find the Kolmogorv-Smirnov probabilities that velocity width, metallicity, dust-to-gas ratio, and Si II equivalent width in the two subsamples are drawn from the same parent population are small. All these quantities are significantly larger in the high cool population, while the H I column densities are indistinguishable in the two populations. We find that heating by X-ray and FUV background radiation is insufficient to balance the cooling rates of either population. Rather, the DLA gas is heated by local radiation fields. The rare appearance of faint, extended objects in the Hubble Ultra Deep Field rules out in situ star formation as the dominant star-formation mode for the high cool population, but is compatible with in situ star formation as the dominant mode for the low cool population. Star formation in the high cool DLAs likely arises in Lyman Break galaxies. We investigate whether these properties of DLAs are analogous to the bimodal properties of nearby galaxies. Using Si II equivalent width as a mass indicator, we construct bivariate distributions of metallicity, lc, and areal SFR versus the mass indicators. Tentative evidence is found for correlations and parallel sequences, which suggest similarities between DLAs and nearby galaxies. We suggest that the transition-mass model provides a plausible scenario for the bimodality we have found. As a result, the bimodality in current galaxies may have originated in DLAs.