Collision strengths and transition probabilities for Co II infrared forbidden lines

We calculate collision strengths and their thermally-averaged Maxwellian values for electron excitation and de-excitation between the fifteen lowest levels of singly-ionised cobalt, Co+, which give rise to emission lines in the near- and mid-infrared. Transition probabilities are also calculated and relative line intensities predicted for conditions typical of supernova ejecta. The diagnostic potential of the 10.52, 15.46 and 14.74 micro-metre transition lines is briefly discussed.Comment: 9 pages, 4 figures, 7 table

Fire in the rain : academic librarians and the new profession of ‘rare book engineering’

Version of RecordPublishe

A Contribution to Reading: The Nebraska Golden Sower Reading/Award Program

Child-choice state book awards are a double-edged sword. On one hand they are popular with children and librarians and they provide an invitation to reading. (Jordan, 1979) On the other hand, they are criticized for being popularity contests with lists of nominees that often overlook the better books. Detractors feel that titles in state book award programs are assumed to be of lesser quality than the national winners such as Newbery or Caldecott books. Opponents also believe that children are incapable of making decisions/judgments regarding literary quality when voting for a state book award winner. (Kaye, 1984) One critic noted that if the matter were food and the children selected \u27Twinkies\u27 over fresh fruit, no nutritionist would be asked to kowtow to the choice. (Gerhardt, 1982) However, inasmuch as there are some 23 state and one regional child-choice award programs, the issue gains importance

Reading Role Models: Fictional Readers in Children\u27s Books

Teachers and librarians know how important reading role models are in fostering a positive attitude toward books. This crucial aspect of a child\u27s education should go beyond decoding and comprehension to encompass a true enjoyment of reading. Educators also hope that youngsters will value literature for what it is and what it has to offer. Such a mind set is frequently incubated at home and further developed early on in the elementary grades

Reading Comprehension, Visual Literacy and Picture Book Illustrations

The books selected for this article demand close inspection of the pictures by readers of varied ages. Children and adults alike will be challenged in the investifations that will lead toward a more comprehensive understanding of illustrations and their value

Spectral variation in the X-ray pulsar GX 1+4 during a low-flux episode

The X-ray pulsar GX 1+4 was observed with the RXTE satellite for a total of 51ks between 1996 July 19 - 21. During this period the flux decreased smoothly from an initial mean level of ~ 6 X 10^36 erg/s to a minimum of ~ 4 X 10^35 erg/s (2-60 keV, assuming a source distance of 10 kpc) before partially recovering towards the initial level at the end of the observation. BATSE pulse timing measurements indicate that a torque reversal took place approximately 10 d after this observation. Both the mean pulse profile and the photon spectrum varied significantly. The observed variation in the source may provide important clues as to the mechanism of torque reversals. The single best-fitting spectral model was based on a component originating from thermal photons with kT ~ 1 keV Comptonised by a plasma of temperature kT \~ 7 keV. Both the flux modulation with phase during the brightest interval and the evolution of the mean spectra over the course of the observation are consistent with variations in this model component; with, in addition, a doubling of the column density nH contributing to the mean spectral change. A strong flare of duration 50 s was observed during the interval of minimum flux, with the peak flux ~ 20 times the mean level. Although beaming effects are likely to mask the true variation in Mdot thought to give rise to the flare, the timing of a modest increase in flux prior to the flare is consistent with dual episodes of accretion resulting from successive orbits of a locally dense patch of matter in the accretion disc.Comment: 8 pages, 3 figures, submitted to MNRA

Observations of far-infrared fine structure lines: o III88.35 micrometer and oI 63.2 micrometer

Observations of the O III 88.35 micrometer line and the O I63.2 micrometer were made with a far infrared spectrometer. The sources M17, NGC 7538, and W51 were mapped in the O III line with 1 arc minute resolution and the emission is found to be quite widespread. In all cases the peak of the emission coincides with the maximum radio continuum. The far infrared continuum was mapped simultaneously and in M17, NGC 7538, and W51 the continuum peak is found to be distinct from the center of ionization. The O III line was also detected in W3, W49, and in a number of positions in the Orion nebula. Upper limits were obtained on NGS 7027, NGC 6572, DR21, G29.9-0.0 and M82. The 63.2 micrometer O I line was detected in M17, M42, and marginally in DR21. A partial map of M42 in this line shows that most of the emission observed arises from the Trapezium and from the bright optical bar to the southeast

Pulse Profiles, Accretion Column Dips and a Flare in GX 1+4 During a Faint State

The Rossi X-ray Timing Explorer (RXTE) spacecraft observed the X-ray pulsar GX 1+4 for a period of 34 hours on July 19/20 1996. The source faded from an intensity of ~20 mCrab to a minimum of <~0.7 mCrab and then partially recovered towards the end of the observation. This extended minimum lasted ~40,000 seconds. Phase folded light curves at a barycentric rotation period of 124.36568 +/- 0.00020 seconds show that near the center of the extended minimum the source stopped pulsing in the traditional sense but retained a weak dip feature at the rotation period. Away from the extended minimum the dips are progressively narrower at higher energies and may be interpreted as obscurations or eclipses of the hot spot by the accretion column. The pulse profile changed from leading-edge bright before the extended minimum to trailing-edge bright after it. Data from the Burst and Transient Source Experiment (BATSE) show that a torque reversal occurred <10 days after our observation. Our data indicate that the observed rotation departs from a constant period with a Pdot/P value of ~-1.5% per year at a 4.5 sigma significance. We infer that we may have serendipitously obtained data, with high sensitivity and temporal resolution about the time of an accretion disk spin reversal. We also observed a rapid flare which had some precursor activity, close to the center of the extended minimum.Comment: 19 pages, 6 figures, accepted for publication in Astrophysical Journal (tentatively scheduled for vol. 529 #1, 20 Jan 2000

Effective communication of software development knowledge through community portals

Knowledge management plays an important role in many software organizations. Knowledge can be captured and distributed using a variety of media, including traditional help files and manuals, videos, technical articles, wikis, and blogs. In recent years, web-based community portals have emerged as an important mechanism for combining various communication channels. However, there is little advice on how they can be effectively deployed in a software project. In this paper, we present a first study of a community portal used by a closed source software project. Using grounded theory, we develop a model that characterizes documentation artifacts along several dimensions, such as content type, intended audience, feedback options, and review mechanisms. Our findings lead to actionable advice for industry by articulating the benefits and possible shortcomings of the various communication channels in a knowledge-sharing portal. We conclude by suggesting future research on the increasing adoption of community portals in software engineering projects.Christoph Treude, Margaret-Anne Stor