The formation of low-ionization emission in the halo of NGC 891

Imaging and Spectroscopic study first revealed the presence of a diffuse ionized medium (DIM), having unusual excitation, pervading the lower halo of the edge-on spiral galaxy NGC 891. Emission from this DIM is strongest northeast of the nucleus, at radii between 2 and 8 kpc (hereafter region 1). The (N2)(lambda)6583/H(alpha) and (S2)(lambda) (lambda)6716,6731/H(alpha) ratios increase dramatically with z in region 1, from 0.6 and 0.5 respectively at z is approximately equal to 500 pc to 1.1 and 1.0 at z is approximately equal to 1 kpc, while nondetections of (O1)(lambda)6300 and (O3)(lambda)5007 emission yield upper limits of (O1)(lambda)6300/H(alpha) less than or equal to 0.05 and (O3)(lambda)5007/H(alpha) less than or equal to 0.15 for z less than 1 kpc. Previous photoionization models, using the radiation field from disk O and B stars, have been successful in reproducing the elevated (N2)(lambda)6583/H(alpha) and (S2)(lambda)(lambda)6716.6731/H(alpha) ratios observed. However, these radiation bounded models also produce significant (O3)(lambda)5007 emission, in conflict with the observed upper limit. Here, we report the results of new, matter bounded models for the photoionization of the DIM in region 1 of NGC 891

Government Drug Testing: A Question of Reasonableness

The 1980s were noted for the escalation of the war on drugs. The dominant public perception was that drug use is a hideous evil that must be stopped, even at a great cost of public resources and personal liberties. Parents, politicians, and law enforcement officials rallied to battle drug use.2 Tremendous expenses and limited victories did not slow the war on drugs.\u27It cannot be disputed that drug abuse is widespread. More than seventy million Americans have experimented with illegal drugs, and twenty-three million currently use an illegal drug.4 The costs to society include drug-related crimes, accidents, lost productivity, increased health costs, and personal suffering.\u27 Drug users\u27 employers bear a large portion of the costs resulting from lost productivity, accidents, illnesses,and related expenses. Some employers have responded by requiring employees to be tested for drug use. The federal government, the Nation\u27s largest employer, is leading the way in drug testing.8 Serious fourth amendment issues arise, however, when the government forces employees to submit to drug testing as a condition of employment. The typical urinalysis of a government employee constitutes a search without a warrant, probable cause, or individualized suspicion that a particular employee violated a law or even a workplace rule. Nevertheless, the United States Supreme Court in 1989 upheld government drug testing programs in National Treasury Employees Union v. Von Raab and Skinner v. Railway Labor Executives\u27 Association.\u27 These cases were among a flood of recent federal and state court decisions allowing mandatory testing of federal, state, and municipal employees and private employees in pervasively regulated industries. These rulings have led several commentators to note that a drug exception to the fourth amendment may be emerging.\u27 Part II of this Note details the executive branch\u27s efforts to per-form drug tests on its employees and on private employees in pervasively regulated industries. Part III traces the Supreme Court\u27s recent erosion of traditional fourth amendment protections against search and seizure. Part IV describes the Supreme Court\u27s analysis of the executive branch\u27s efforts at drug testing. Part V examines the analytical structure that courts use to determine the constitutionality of drug testing by the government. Part VI traces judicial trends in unsettled legal areas. Finally, Part VII concludes that the Court\u27s reasonableness balancing test provides no concrete limit on government searches

Influence of the active nucleus on the multiphase interstellar medium in NGC 1068

The luminous spiral NGC 1068 has now been imaged from x-ray to radio wavelengths at comparably high resolution (approximately less than 5 in. FWHM). The bolometric luminosity of this well-known Seyfert is shared almost equally between the active nucleus and an extended 'starburst' disk. In an ongoing study, we are investigating the relative importance of the nucleus and the disk in powering the wide range of energetic activity observed throughout the galaxy. Our detailed analysis brings together a wealth of data: ROSAT HRI observations, VLA lambda lambda 6-20 cu cm and OVRO interferometry, lambda lambda 0.4-10.8 micron imaging, and Fabry-Perot spectrophotometry

Reframing the Fields

The conception of metaphoric process elaborated by Mary Gerhart and Allan Russell illuminates a key mechanism often involved in the most significant advances in science and religion. Attention to this conceptual device provides a productive way to reframe the relationships and dialogues between the fields. The theory has compelling implications for reframing the understanding of theology and its task

Hubungan Empati Petani Dan Keterampilan Sebagai Fasilitator Di Pusat Pelatihan Pertanian Dan Pedesaan Swadaya Jawa Barat

Tujuan penelitian adalah menganalisis hubungan empati petani dan keterampilan sebagai fasilitator pembelajaran bagi para petani di Pusat Pelatihan Pertanian Swadaya (P4S). Jenis penelitian adalah survei dengan melibatkan 140 orang petani fasilitator P4S di 17 kabupaten, Provinsi Jawa Barat sebagai responden. Sebanyak 86,43% responden memiliki empati dalam kategori sedang dan 13,57% berada dalam kategori tinggi. Sebanyak 54,29% responden memiliki keterampilan memfasilitasi berada dalam kategori tinggi dan 45,71% dalam kategori sedang. Analisis korelasional menunjukkan bahwa terdapat hubungan positif yang signifikan antara empati dan keterampilan memfasilitasi (p<0,05) dengan derajat hubungan yang lemah (r=0,02)

A targeted search for repeating fast radio bursts with the MWA

We present a targeted search for low-frequency (144--215\,MHz) FRB emission from five repeating FRBs using 23.3\,hr of archival data taken with the Murchison Widefield Array (MWA) Voltage Capture System (VCS) between 2014 September and 2020 May. This is the first time that the MWA VCS has been used to search for FRB signals from known repeaters, which enables much more sensitive FRB searches than previously performed with the standard MWA correlator mode. We performed a standard single pulse search with a temporal and spectral resolution of $400\,\mu$s and 10\,kHz, respectively, over a $100\,\text{pc}\,\text{cm}^{-3}$ dispersion measure (DM) range centred at the known DM of each studied repeating FRB. No FRBs exceeding a $6\sigma$ threshold were detected. The fluence upper limits in the range of 32--1175\,Jy\,ms and 36--488\,Jy\,ms derived from 10 observations of FRB 20190711A and four observations of FRB 20201124A respectively, allow us to constrain the spectral indices of their bursts to $\gtrsim-1$ if these two repeaters were active during the MWA observations. If free-free absorption is responsible for our non-detection, we can constrain the size of the absorbing medium in terms of the electron temperature $T$ to $<1.00\times(T/10^4\text{K})^{-1.35}\,\text{pc}$, $<0.92\times(T/10^4\text{K})^{-1.35}\,\text{pc}$ and $<[0.22\text{--}2.50]\times(T/10^4\text{K})^{-1.35}\,\text{pc}$ for FRB 20190117A, 20190711A, and 20201124A, respectively. However, given that the activities of these repeaters are not well characterised, our non-detections could also suggest they were inactive during the MWA observations.Comment: Accepted for publication in MNRA

The State of the Region: Hampton Roads 2012

This is Old Dominion University\u27s 13th annual State of the Region Report. While it represents the work of many people connected in various ways to the university, the report does not constitute an official viewpoint of Old Dominion or it\u27s president, John R. Broderick. The report maintains the goal of stimulating thought and discussion that ultimately will make Hampton Roads an even better place to live. We are proud of our region\u27s many successes, but realize that it is possible to improve our performance. In order to do so, we must have accurate information about where we are and a sound understanding of the policy options open to us.https://digitalcommons.odu.edu/economics_books/1006/thumbnail.jp

Murchison Widefield Array rapid-response observations of the short GRB 180805A

Abstract Here we present stringent low-frequency (185 MHz) limits on coherent radio emission associated with a short-duration gamma-ray burst (SGRB). Our observations of the short gamma-ray burst (GRB) 180805A were taken with the upgraded Murchison Widefield Array (MWA) rapid-response system, which triggered within 20s of receiving the transient alert from the Swift Burst Alert Telescope, corresponding to 83.7 s post-burst. The SGRB was observed for a total of 30 min, resulting in a $3\sigma$ persistent flux density upper limit of 40.2 mJy beam–1. Transient searches were conducted at the Swift position of this GRB on 0.5 s, 5 s, 30 s and 2 min timescales, resulting in $3\sigma$ limits of 570–1 830, 270–630, 200–420, and 100–200 mJy beam–1, respectively. We also performed a dedispersion search for prompt signals at the position of the SGRB with a temporal and spectral resolution of 0.5 s and 1.28 MHz, respectively, resulting in a $6\sigma$ fluence upper-limit range from 570 Jy ms at DM $=3\,000$ pc cm–3 ( $z\sim 2.5$ ) to 1 750 Jy ms at DM $=200$ pc cm–3 ( $z\sim 0.1)$ , corresponding to the known redshift range of SGRBs. We compare the fluence prompt emission limit and the persistent upper limit to SGRB coherent emission models assuming the merger resulted in a stable magnetar remnant. Our observations were not sensitive enough to detect prompt emission associated with the alignment of magnetic fields of a binary neutron star just prior to the merger, from the interaction between the relativistic jet and the interstellar medium (ISM) or persistent pulsar-like emission from the spin-down of the magnetar. However, in the case of a more powerful SGRB (a gamma-ray fluence an order of magnitude higher than GRB 180805A and/or a brighter X-ray counterpart), our MWA observations may be sensitive enough to detect coherent radio emission from the jet-ISM interaction and/or the magnetar remnant. Finally, we demonstrate that of all current low- frequency radio telescopes, only the MWA has the sensitivity and response times capable of probing prompt emission models associated with the initial SGRB merger event.</jats:p

Self-regulation and the foraging gene (PRKG1) in humans

We would like to thank Dr. Sara Mostafavi (University of British Columbia) for directing us to the CMC website regarding gene expression for rs13499 and for statistical advice. This work was supported by NSERC Discovery funds to JD and a Canadian Institute for Advanced Research award to MS.Peer reviewedPostprin

The State of the Region: Hampton Roads 2006

This is Old Dominion University\u27s seventh annual State of the Region report. While it represents the work of many people connected in various ways to the university, the report does not constitute an official viewpoint of Old Dominion, or it\u27s president, Roseann Runte. The report maintains the goal of stimulating thought and discussion that ultimately will make Hampton Roads an even better place to live. We are proud of our region\u27s many successes, but realize that it is possible to improve our performance. In order to do so, we must have accurate information about where we are and a sound understanding of the policy options open to us.https://digitalcommons.odu.edu/economics_books/1012/thumbnail.jp