The environmental dependence of neutral hydrogen content in spiral galaxies

We present a study of the relationship between the deficiency of neutral hydrogen and the local three-dimensional number density of spiral galaxies in the Arecibo catalog of global HI measurements (Springob et al. 2005). We find that the dependence on density of the HI content is weak at low densities, but increases sharply at high densities where interactions between galaxies and the intra-cluster medium become important. This behavior is reminiscent of the morphology-density relation (Dressler 1980) in that the effect manifests itself only at cluster-type densities, and indeed when we plot both the HI deficiency-density and morphology-density relations, we see that the densities at which they "turn up" are similar. This suggests that the physical mechanisms responsible for the increase in early types in clusters are also responsible for the decrease in HI content.Comment: To appear in AIP Conference Proceedings, "The Evolution of Galaxies through the Neutral Hydrogen Window", Feb 1-3 2008, Arecibo, Puerto Rico, eds. R. Minchin & E. Momjian. 3 pages, 2 figure

Development of Near-Infrared Spectroscopic Chronometers for Galaxy Evolution: Critical Testing With Nearby Galaxies

I present preliminary results in the development of a near-infrared (NIR) spectroscopic chronometer for studying stellar populations in galaxies. By examining NIR IRTF/SpeX spectroscopy of the young post-starburst galaxy NGC 5102, and the compact elliptical M32, I have defined six indices that measure the strength of features due to thermally-pulsing asymptotic giant branch (TP-AGB) and main sequence turn-off (MSTO) stars, which are prominent in the integrated spectra of young populations. Two indices measure equivalent widths of Paschen lines originating in the atmospheres of hot stars, and are sensitive to ages up to ~100 Myr; three indices measure the flux ratios of narrow bands surrounding molecular absorption breaks due to very cool and luminous TP-AGB stars; and the final index is a blended line also sensitive to TP-AGB stars. The TP-AGB is known to dominate the NIR flux of stellar populations between ~100 Myr and 3 Gyr, and therefore the indices are particularly sensitive to ages in this regime. To demonstrate that the NIR indices can be used as chronometers, I compare the values measured in NGC~5102 and M32 to those in the Maraston (2005) stellar population models for a grid of ages and metallicities. The model-derived star formation histories for both galaxies are consistent with previous studies with established optical spectroscopic techniques. Moreover, in the case of NGC~5102 the indices are able to detect the presence of two distinct stellar populations with ages ~20-40 Myr and several hundred Myr. I also address the issue of TP-AGB contribution in stellar population models, which is largely uncertain due to poorly understood processes in the evolution of TP-AGB stars, such as mass loss and convective burning. I find that the TP-AGB contribution in the Maraston (2005) models is accurate within error limits on the measured indices. Therefore, more work will be needed to place strict limits on this important ingredient in stellar population models. The NIR indices in M32 are also examined, and model comparisons predict an SSP-equivalent age of ~2.75 Gyr, consistent with optical studies. A more complicated star formation history in M32 cannot be ruled out, however, because the sensitivity of the indices declines at intermediate ages

STAR FORMATION IN PARTIALLY GAS-DEPLETED SPIRAL GALAXIES

Broadband B and R and H-alpha images have been obtained with the 4.1-m SOAR telescope atop Cerro Pachon, Chile for 29 spiral galaxies in the Pegasus I galaxy cluster and for 18 spirals in non-cluster environments. Pegasus I is a spiral-rich cluster with a low density intracluster medium and a low galaxy velocity dispersion. When combined with neutral hydrogen (HI) data obtained with the Arecibo 305-m radiotelescope, acquired by Levy et al. (2007) and by Springob et al. (2005a), we study the star formation rates in disk galaxies as a function of their HI deficiency. To quantify HI deficiency, we use the usual logarithmic deficiency parameter, DEF. The specific star formation rate (SSFR) is quantified by the logarithmic flux ratio of H-alpha flux to R band flux, and thus roughly characterizes the logarithmic SFR per unit stellar mass. We find a clear correlation between the global SFR per unit stellar mass and DEF, such that the SFR is lower in more HI-deficient galaxies. This correlation appears to extend from the most gas-rich to the most gas-poor galaxies. We also find a correlation between the central SFR per unit mass relative to the global values, in the sense that the more HI-deficient galaxies have a higher central SFR per unit mass relative to their global SFR values than do gas-rich galaxies. In fact, approximately half of the HI-depleted galaxies have highly elevated SSFRs in their central regions, indicative of a transient evolutionary state. In addition, we find a correlation between gas-depletion and the size of the H-alpha disk (relative to the R band disk); HI-poor galaxies have truncated disks. Moreover, aside from the elevated central SSFR in many gas-poor spirals, the SSFR is otherwise lower in the H-alpha disks of gas-poor galaxies than in gas-rich spirals

Coordinate control of axon defasciculation and myelination by laminin-2 and -8

Schwann cells form basal laminae (BLs) containing laminin-2 (Ln-2; heterotrimer α2β1γ1) and Ln-8 (α4β1γ1). Loss of Ln-2 in humans and mice carrying α2-chain mutations prevents developing Schwann cells from fully defasciculating axons, resulting in partial amyelination. The principal pathogenic mechanism is thought to derive from structural defects in Schwann cell BLs, which Ln-2 scaffolds. However, we found loss of Ln-8 caused partial amyelination in mice without affecting BL structure or Ln-2 levels. Combined Ln-2/Ln-8 deficiency caused nearly complete amyelination, revealing Ln-2 and -8 together have a dominant role in defasciculation, and that Ln-8 promotes myelination without BLs. Transgenic Ln-10 (α5β1γ1) expression also promoted myelination without BL formation. Rather than BL structure, we found Ln-2 and -8 were specifically required for the increased perinatal Schwann cell proliferation that attends myelination. Purified Ln-2 and -8 directly enhanced in vitro Schwann cell proliferation in collaboration with autocrine factors, suggesting Lns control the onset of myelination by modulating responses to mitogens in vivo

Differential cross section measurements for the production of a W boson in association with jets in proton–proton collisions at √s = 7 TeV

Measurements are reported of differential cross sections for the production of a W boson, which decays into a muon and a neutrino, in association with jets, as a function of several variables, including the transverse momenta (pT) and pseudorapidities of the four leading jets, the scalar sum of jet transverse momenta (HT), and the difference in azimuthal angle between the directions of each jet and the muon. The data sample of pp collisions at a centre-of-mass energy of 7 TeV was collected with the CMS detector at the LHC and corresponds to an integrated luminosity of 5.0 fb[superscript −1]. The measured cross sections are compared to predictions from Monte Carlo generators, MadGraph + pythia and sherpa, and to next-to-leading-order calculations from BlackHat + sherpa. The differential cross sections are found to be in agreement with the predictions, apart from the pT distributions of the leading jets at high pT values, the distributions of the HT at high-HT and low jet multiplicity, and the distribution of the difference in azimuthal angle between the leading jet and the muon at low values.United States. Dept. of EnergyNational Science Foundation (U.S.)Alfred P. Sloan Foundatio