Exile Vol. XLV No. 2

43rd Year Title Page 3 Epigraph by Ezra Pound 5 Table of Contents 7 Contributors Notes 74-75 Editorial Board 76 INTERVIEWS The Art of Hearing: Interview with Stanley Plumly by Alison Stine \u2700 23-27 ART Self-Portrait by Angela Bliss \u2799 8 For a Living by Angela Bliss \u2799 12 Untitled by Frazier Taylor \u2702 22 Untitled by Amy Deaner \u2799 29 Perfect Knee by David Tulkin \u2701 34 Untitled by Amy Deaner \u2799 43 Still Light by Angela Bliss \u2799 62 Hiding Nature by Amy Deaner \u2799 64 Self-Portrait A by Sarah Leyrer \u2701 73 POETRY Bolted Back by Michelle Grindstaff \u2702 9 Squall by Georgia Riepe \u2702 10 Loaves and Fishes by Maeghan Demmons \u2701 11 World Cafe by Katie Kroner \u2701 28 Gurney Surfer by Tom Hankinson \u2702 31 Japanese Beetles by Alison Stine \u2700 32-33 Shoveling by Bekah Taylor \u2700 40 Tobacco Country by K. Moore \u2701 41 Winton Place by Rachel Colina \u2702 42 Bottom of the Ninth by Michelle Grindstaff \u2702 61 Fall Burning by Alison Stine \u2700 63 rocking by Bekah Taylor \u2700 71 The Armor of the Beach by Georgia Riepe \u2702 72 PROSE In the Aisles of the Night by Tom Dussel \u2701 13-21 From Those Uninvolved by Justin Walker \u2799 30 Frame by Paul Durica \u2700 35-39 The Rose by Rachel Bolton \u2799 44-60 Stop at the Soldier by Hillary Campbell \u2700 65-70 All submissions are reviewed on an anonymous basis, and all editorial decisions are shared equally among the members of the Editorial Board. -76 Cover Art Untitled by Kris Lewis \u2799 / Back Cover Art Figure 25 by Todd Gys \u2799 -76 Printed by Printing Arts Press -7

Exile Vol. XLVIII

46th Year Title Page 3 Epigraph by Ezra Pound 5 Table of Contents 7 Contributors\u27 Notes 59-60 Editorial Board 61 ART Connected by Christin Faison \u2704 8 Marcya by Harper Leich \u2704 12 Untitled by Derek Mong \u2704 19 Epistemological Torment by Matthew Sove \u2704 21 Consummatum Est I by Matthew Sove \u2704 27 Consummatum Est III by Matthew Sove \u2704 29 The Sheraton by Harper Leich \u2704 39 Untitled by Roman Sehling \u2703 43 My War by Matthew Sove \u2704 53 POETRY Chores, Then and Now by Dan Rohrer \u2704 9 Heaven by Chris Million \u2702 10-11 Loving her in Balinese by Ginna Fuselier \u2703 20 The Shower Room by Derek Mong \u2704 28 The Wailua by Jenny Silva \u2702 40-41 Good to the Last Drop by Chrissy Swinko \u2703 42 PROSE The House of Spider Webs by Dianna Craig \u2703 13-18 The Golem by Owen McGrann \u2703 22-26 All the String in Cincinnati by Rachel Colina \u2702 30-38 Passing by Matthew Martz \u2702 44-52 True War Story by Dianna Craig \u2703 54-58 All submissions are reviewed on an anonymous basis, and all editorial decisions are shared equally among the members of the Editorial Board. -61 Cover Art Out to Dry by Thomas DeCarlo \u2705 / Back Cover Art Untitled by Thomas DeCarlo \u2705 -61 Printing by Printing Arts Press -6

Differences between CO- and calcium triplet-derived velocity dispersions in spiral galaxies: evidence for central star formation?

We examine the stellar velocity dispersions (sigma) of a sample of 48 galaxies, 35 of which are spirals, from the Palomar nearby galaxy survey. It is known that for ultra-luminous infrared galaxies (ULIRGs) and merger remnants thesigma derived from the near-infrared CO band-heads is smaller than that measured from optical lines, while no discrepancy between these measurements is found for early-type galaxies. No such studies are available for spiral galaxies - the subject of this paper. We used cross-dispersed spectroscopic data obtained with the Gemini Near-Infrared Spectrograph (GNIRS), with spectral coverage from 0.85 to 2.5um, to obtain sigma measurements from the 2.29 $\mu$m CO band-heads (sigma_{CO}), and the 0.85 um calcium triplet (sigma_{CaT}). For the spiral galaxies in the sample, we found that sigma_{CO} is smaller than sigma_{CaT}, with a mean fractional difference of 14.3%. The best fit to the data is given by sigma_{opt} = (46.0+/-18.1) + (0.85+/-0.12)sigma_{CO}. This "sigma discrepancy" may be related to the presence of warm dust, as suggested by a slight correlation between the discrepancy and the infrared luminosity. This is consistent with studies that have found no sigma-discrepancy in dust-poor early-type galaxies, and a much larger discrepancy in dusty merger remnants and ULIRGs. That sigma_{CO}$ is lower than sigma_{opt} may also indicate the presence of a dynamically cold stellar population component. This would agree with the spatial correspondence between low sigma_{CO} and young/intermediate-age stellar populations that has been observed in spatially-resolved spectroscopy of a handful of galaxies.Comment: Published in MNRAS, 446, 282

Physical properties of Herschel selected galaxies in a semi-analytic galaxy formation model

[Abridged] We make use of a semi-analytic cosmological model that includes simple prescriptions for dust attenuation and emission to make predictions for the observable and physical properties of galaxies that may be detected by the recently launched Herschel Space Observatory in deep fields such as GOODS-Herschel. We compare our predictions for differential galaxy number counts in the PACS (100 & 160) and SPIRE (250, 350, and 500 micron) bands with available observations. We find very good agreement with the counts in the PACS bands, for the overall counts and for galaxies binned by redshift at z< 2. At z > 2 our model underpredicts the number of bright galaxies by a factor of ten. The agreement is much worse for all three SPIRE bands, and becomes progressively worse with increasing wavelength. We discuss a number of possible reasons for these discrepancies, and hypothesize that the effect of blending on the observational flux estimates is likely to be the dominant issue. We note that the PACS number counts are relatively robust to changes in the dust emission templates, while the predicted SPIRE number counts are more template dependent. We present quantitative predictions for the relationship between the observed PACS 160 and SPIRE 250 micron fluxes and physical quantities such as halo mass, stellar mass, cold gas mass, star formation rate, and total infrared (IR) luminosity, at different redshifts. We also present quantitative predictions for the correlation between PACS 160 micron flux and the probability that a galaxy has experienced a recent major or minor merger. Although our models predict a strong correlation between these quantities, such that more IR-luminous galaxies are more likely to be merger-driven, we find that more than half of all high redshift IR-luminous galaxies detected by Herschel are able to attain their high star formation rates without enhancement by a merger.Comment: Accepted for publication in MNRA

A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei

We present a new semi-analytic model that self-consistently traces the growth of supermassive black holes (BH) and their host galaxies within the context of the LCDM cosmological framework. In our model, the energy emitted by accreting black holes regulates the growth of the black holes themselves, drives galactic scale winds that can remove cold gas from galaxies, and produces powerful jets that heat the hot gas atmospheres surrounding groups and clusters. We present a comprehensive comparison of our model predictions with observational measurements of key physical properties of low-redshift galaxies, such as cold gas fractions, stellar metallicities and ages, and specific star formation rates. We find that our new models successfully reproduce the exponential cutoff in the stellar mass function and the stellar and cold gas mass densities at z~0, and predict that star formation should be largely, but not entirely, quenched in massive galaxies at the present day. We also find that our model of self-regulated BH growth naturally reproduces the observed relation between BH mass and bulge mass. We explore the global formation history of galaxies in our models, presenting predictions for the cosmic histories of star formation, stellar mass assembly, cold gas, and metals. We find that models assuming the "concordance" LCDM cosmology overproduce star formation and stellar mass at high redshift (z>2). A model with less small-scale power predicts less star formation at high redshift, and excellent agreement with the observed stellar mass assembly history, but may have difficulty accounting for the cold gas in quasar absorption systems at high redshift (z~3-4).Comment: MNRAS accepte

The James Webb Space Telescope Mission

Twenty-six years ago a small committee report, building on earlier studies, expounded a compelling and poetic vision for the future of astronomy, calling for an infrared-optimized space telescope with an aperture of at least $4m$. With the support of their governments in the US, Europe, and Canada, 20,000 people realized that vision as the $6.5m$ James Webb Space Telescope. A generation of astronomers will celebrate their accomplishments for the life of the mission, potentially as long as 20 years, and beyond. This report and the scientific discoveries that follow are extended thank-you notes to the 20,000 team members. The telescope is working perfectly, with much better image quality than expected. In this and accompanying papers, we give a brief history, describe the observatory, outline its objectives and current observing program, and discuss the inventions and people who made it possible. We cite detailed reports on the design and the measured performance on orbit.Comment: Accepted by PASP for the special issue on The James Webb Space Telescope Overview, 29 pages, 4 figure

The complex, dusty narrow-line region of NGC 4388 : gas–jet interactions, outflows and extinction revealed by near-IR spectroscopy

We present Gemini/GNIRS (Gemini Near-Infrared Spectrograph) spectroscopy of the Seyfert 2 galaxy NGC 4388, with simultaneous coverage from 0.85 to 2.5 μm. Several spatially extended emission lines are detected for the first time, both in the obscured and unobscured portion of the optical narrow-line region (NLR), allowing us to assess the combined effects of the central continuum source, outflowing gas and shocks generated by the radio jet on the central 280 pc gas. The HI and [Fe II] lines allow us to map the extinction affecting the NLR. We found that the nuclear region is heavily obscured, with E(B − V) ∼ 1.9 mag. To the NE of the nucleus and up to ∼150 pc, the extinction remains large, ∼1 mag or larger, consistent with the system of dust lanes seen in optical imaging.We derived position–velocity diagrams for the most prominent lines as well as for the stellar component. Only the molecular gas and the stellar component display a well-organized pattern consistent with disc rotation. Other emission lines are kinematically perturbed or show little evidence of rotation. Extended high-ionization emission of sulphur, silicon and calcium is observed to distances of at least 200 pc both NE and SW of the nucleus. We compared flux ratios between these lines with photoionization models and conclude that radiation from the central source alone cannot explain the observed high-ionization spectrum. Shocks between the radio jet and the ambient gas are very likely an additional source of excitation. We conclude that NGC 4388 is a prime laboratory to study the interplay between all these mechanisms