1,726,583 research outputs found
[Cambria Steel Co., Engine Drawing Card, Sketch No. 6902]
No full textThis engine drawing card was created for the Cambria and Indiana Railroad, Class 8-44 E. Section J-8E. Sketch 6902. Copy Spec. C-6325
Linked collectors and determiners for: UF Florida Museum Paleobotany.
No full textNatural history specimen data linked to collectors and determiners held within, "UF Florida Museum Paleobotany". Claims or attributions were made on Bionomia by volunteer Scribes, <a href="http://bionomia.net/dataset/5f0d32a4-6902-481b-9694-6393ad40b973">https://bionomia.net/dataset/5f0d32a4-6902-481b-9694-6393ad40b973</a> using specimen data from the dataset aggregated by the Global Biodiversity Information Facility, <a href="https://gbif.org/dataset/5f0d32a4-6902-481b-9694-6393ad40b973">https://gbif.org/dataset/5f0d32a4-6902-481b-9694-6393ad40b973</a>. Formatted as a Frictionless Data package
California Poll: 6902 -- May 1-4, 1969
No full textThe Field Poll, established in 1945 as The California Poll by Mervin Field, has operated continuously as an independent, non-partisan, media-sponsored public opinion news service. Each year the Field Polls cover a wide range of political and social topics examining California public opinion. Continuing measures are made of voter support for leading political figures vying for major state and federal offices, job ratings of important political figures and reactions to significant political events. Voter awareness, understanding and predispositions of major campaign issues and salient statewide ballot propositions are also tracked over time. For poll 6902 N=1011
Radio-continuum observations of small, radially polarised Supernova Remnant J0519-6902 in the large Magellanic cloud
No full textWe report on new Australian Telescope Compact Array (ATCA) observations of SNR J0519-6902. The Supernova Remnant (SNR) is small in size (~8 pc) and exhibits a typical SNR spectrum of alpha = -0.53 ± 0.07, with steeper spectral indices found towards the northern limb of the remnant. SNR J0519-6902 contains a low level of radially orientated polarisation at wavelengths of 3 & 6 cm, which is characteristic of younger SNRs. A fairly strong magnetic field was estimated of ~171 microG. The remnant appears to be the result of a typical Type Ia supernovae, sharing many properties as another small and young Type Ia LMC SNR, J0509-6731
Going Beyond Counting First Authors in Author Co-citation Analysis
No full textThe present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
The warm circumstellar envelope and wind of the G9 IIb star HR 6902
No full textIUE observations of the eclipsing binary system
HR 6902 obtained at various epochs spread over four years indicate
the presence of warm circumstellar material enveloping the G9 IIb
primary. The spectra show Sii
A new radio continuum study of the large magellanic cloud supernova remnant MC SNR J0519–6902
No full textInternational audienceWe present a new radio continuum study of the Large Magellanic Cloud supernova remnant (SNR) MC SNR J0519-6902. With a diameter of ∼8 pc, this SNR shows a radio ring-like morphology with three bright regions towards the north, east, and south. Its linear polarisation is prominent with average values of 5 ± 1% and 6 ± 1% at 5 500 and 9 000 MHz, and we find a spectral index of -0.62 ± 0.02, typical of a young SNR. The average rotation measure is estimated at -124 ± 83 rad m -2 and the magnetic field strength at ∼ 11 μG. We also estimate an equipartition magnetic field of 72 ± 5 μG and minimum explosion energy of E min = 2.6×10 48 erg. Finally, we identified an H I cloud that may be associated with MC SNR J0519-6902, located in the southeastern part of the remnant, along with a potential wind-bubble cavity.</div
Pilot survey for Lyme disease antibodies in Brisbane dogs
No full textID: 6902; LR: 20031114; JID: 0370616; 0 (Antibodies, Bacterial); ppublis
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