The Lasting Impacts of the NICU Experience and How a Community Supports the Premature Infant and Their Family

Every year, approximately 500,000 babies in the United States are born before 37 weeks gestation. Often premature birth results in a stay in the Neonatal Intensive Care Unit (NICU) for some length of time. A literature review shows that there are lasting impacts on both the parents and the premature infant due to a stay in the NICU. These impacts can affect the parents’ mental health, the attachment between parents and infant, and the infant’s overall development for years to come. Findings from two qualitative questionnaires completed by previous parents of infants who stayed in the St. Cloud Hospital Neonatal Intensive Care Unit, and St. Cloud area agencies show how the St. Cloud community supports the parents and the premature infant after discharge from the NICU. The parents shared that the biggest support while in the NICU was the March of Dimes, but after discharge, there was limited support from previous supports or local agencies. With limited responses to the questionnaire from local agencies, it became apparent that it may be difficult to get into contact with the agencies. These findings showed the disconnect between supports while in the NICU and supports once discharged from the NICU. The connection between the St. Cloud Hospital NICU and local agencies needs to be an item of focus to increase support for parents and infants born prematurely

Mouse maps of gene expression in the brain

Comprehensive atlases of gene expression in the mouse brain will provide a great resource for neurobiology

High Resolution Spectroscopy of the Pulsating White Dwarf G29-38

We present the analysis of time-resolved, high resolution spectra of the cool white dwarf pulsator, G29-38. From measuring the Doppler shifts of the H-alpha core, we detect velocity changes as large as 16.5 km/s and conclude that they are due to the horizontal motions associated with the g-mode pulsations on the star. We detect seven pulsation modes from the velocity time-series and identify the same modes in the flux variations. We discuss the properties of these modes and use the advantage of having both velocity and flux measurements of the pulsations to test the convective driving theory proposed for DAV stars. Our data show limited agreement with the expected relationships between the amplitude and phases of the velocity and flux modes. Unexpectedly, the velocity curve shows evidence for harmonic distortion, in the form of a peak in the Fourier transform whose frequency is the exact sum of the two largest frequencies. Combination frequencies are a characteristic feature of the Fourier transforms of light curves of G29-38, but before now have not been detected in the velocities, nor does published theory predict that they should exist. We compare our velocity combination frequency to combination frequencies found in the analysis of light curves of G29-38, and discuss what might account for the existence of velocity combinations with the properties we observe. We also use our high-resolution spectra to determine if either rotation or pulsation can explain the truncated shape observed for the DAV star's line core. We are able to eliminate both mechanisms: the average spectrum does not fit the rotationally broadened model and the time-series of spectra provides proof that the pulsations do not significantly truncate the line.Comment: 24 pages, 9 figures, Accepted for publication in ApJ (June

Evidence For Temperature Change And Oblique Pulsation From Light Curve Fits Of The Pulsating White Dwarf GD 358

Convective driving, the mechanism originally proposed by Brickhill for pulsating white dwarf stars, has gained general acceptance as the generic linear instability mechanism in DAV and dbV white dwarfs. This physical mechanism naturally leads to a nonlinear formulation, reproducing the observed light curves of many pulsating white dwarfs. This numerical model can also provide information on the average depth of a star's convection zone and the inclination angle of its pulsation axis. In this paper, we give two sets of results of nonlinear light curve fits to data on the dbV GD 358. Our first fit is based on data gathered in 2006 by the Whole Earth Telescope; this data set was multiperiodic containing at least 12 individual modes. Our second fit utilizes data obtained in 1996, when GD 358 underwent a dramatic change in excited frequencies accompanied by a rapid increase in fractional amplitude; during this event it was essentially monoperiodic. We argue that GD 358's convection zone was much thinner in 1996 than in 2006, and we interpret this as a result of a short-lived increase in its surface temperature. In addition, we find strong evidence of oblique pulsation using two sets of evenly split triplets in the 2006 data. This marks the first time that oblique pulsation has been identified in a variable white dwarf star.Delaware Asteroseismic Research CenterNational Science Foundation AST-0909107, AST-0607840Norman Hackerman Advanced Research Program 003658-0255-2007Crystal Trust FoundationMt. Cuba ObservatoryUniversity of DelawareAstronom

UAS Literary & Arts Journal

Proof copy provided by Tidal Echoes.Featuring the work of students, faculty, and staff of the University of Alaska Southeast and members of the community.A Note from Loren, Sometimes Known as Senior Editor -- A Letter from Josh, Affectionately Known as “Sugah” (say it with a southern accent) -- A Note from Emily Wall -- On the Move -- Dangly Jangly Things -- Taco Surf -- Midwestern Trash -- On the Distaff Side -- Christmas Joy -- The Three Little McCormicks -- Trollin’ Ray’s Brain: An Interview with Ray Troll -- His Long Coat Turning -- First Autumn -- Pinta Cove Birthday Gifts -- September Wings -- When in Rome -- Early Morning Conspiracy Theory -- Flesh Wound -- Two Ravens, Five Ways -- Shades of Brown: The Question -- Hayfield-Clarke Psychiatric Center -- Hardscrabble -- Smoked Meat Sandwiches -- Slime Squishing Through Gold: An Interview with Nora Marks Dauenhauer -- Berries -- Buds -- Grandpa Jakwteen in Eclipse -- Cross Talk -- Voices -- Trouble -- Flying Home -- Snorkeling at Hanauma Bay -- Genocide -- Raven, Saving It for Later -- Mama Abel’s -- Settling In -- Blue -- Dad at 27 -- Dad photographs mother -- Backyard theatre & Oz -- Love-in, Easter Day, 1968 -- Topanga Corral -- Swallowing Senora -- Keeping Time on the Kee Nax Trail -- Ode to Ching -- Beneath the Surface (chapter title) -- A Visit from the Wild -- Teacher’s Pets -- Centennial -- See Spot Rot -- With Salsa -- Moonbaby -- The Fine Art of Raising a Tarpaulin -- Prologue -- Epiphany 2008 -- View of Auke Lake -- Shark Fins -- Translating Pasternak -- Raven Boys -- Institutional Back Door -- Uneasy Disguise -- Christmas Wind -- The Life and Times of the Orlando Bloom Fan Club -- Writer & Artist Biographie

First Results from the Swarms Survey. SDSS 1257+5428: A Nearby, Massive White Dwarf Binary with a Likely Neutron Star or Black Hole Companion

We present the first results from SWARMS (Sloan White dwArf Radial velocity data Mining Survey), an ongoing project to identify compact white dwarf (WD) binaries in the spectroscopic catalog of the Sloan Digital Sky Survey. The first object identified by SWARMS, SDSS 1257+5428, is a single-lined spectroscopic binary in a circular orbit with a period of 4.56 hr and a semiamplitude of 322.7+-6.3 km/s. From the spectrum and photometry, we estimate a WD mass of 0.92(+0.28,-0.32) Msun. Together with the orbital parameters of the binary, this implies that the unseen companion must be more massive than 1.62(+0.20,-0.25) Msun, and is in all likelihood either a neutron star or a black hole. At an estimated distance of 48(+10,-19) pc, this would be the closest known stellar remnant of a supernova explosion.Comment: 8 pages, 8 figures, ApJ in pres

The Peculiar Pulsations of PY Vul

The pulsating white dwarf star PY Vul (G~185-32) exhibits pulsation modes with peculiar properties that set it apart from other variable stars in the ZZ Ceti (DAV) class. These peculiarities include a low total pulsation amplitude, a mode with bizarre amplitudes in the ultraviolet, and a mode harmonic that exceeds the amplitude of its fundamental. Here, we present optical, time series spectroscopy of PY Vul acquired with the Keck II LRIS spectrograph. Our analysis has revealed that the mode with unusual UV amplitudes also has distinguishing characteristics in the optical. Comparison of its line profile variations to models suggests that this mode has a spherical degree of four. We show that all the other peculiarities in this star are accounted for by a dominant pulsation mode of l=4, and propose this hypothesis as a solution to the mysteries of PY Vul.Comment: 30 pages, 14 figures, Accepted for publication in Ap

Pulsational Mapping of Calcium Across the Surface of a White Dwarf

We constrain the distribution of calcium across the surface of the white dwarf star G29-38 by combining time series spectroscopy from Gemini-North with global time series photometry from the Whole Earth Telescope. G29-38 is actively accreting metals from a known debris disk. Since the metals sink significantly faster than they mix across the surface, any inhomogeneity in the accretion process will appear as an inhomogeneity of the metals on the surface of the star. We measure the flux amplitudes and the calcium equivalent width amplitudes for two large pulsations excited on G29-38 in 2008. The ratio of these amplitudes best fits a model for polar accretion of calcium and rules out equatorial accretion.Comment: Accepted to the Astrophysical Journal. 16 pages, 10 figures