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Parisinus graecus 2649 – Pr
No full textThis article provides a codicological and historical description of the manuscript Parisinus graecus 2649, containing the text of Pollux’s Onomasticon
Decreto No. 2649 de 1953
No full textContiene el texto completo del Decreto No. 2649 de 1953 por el cual se reglamenta el decreto extraordinario número 2064 de 1953, orgánico de la Judicatura Municipal
Wreckage of engine #2649, Revelstoke
No full textWreckage of steam engine #2649 in Revelstoke yard. Three unidentified men posing for photo beside engine
Wreck of steam engine #2649, Lethbridge
No full textSteam engine No. 2649 train wreck somewhere between Lethbridge and Nelson
Chicago, Rock Island & Pacific (RI) 2649
No full textA photograph print showing the Chicago, Rock Island & Pacific (CRIP, RI, or ROCK) 2649, 2-8-2, Kansas City, KS
Wreck of steam engine #2649, Nelson
No full textSteam engine #2649 that was involved in train wreck between Nelson and Lethbridge
Block Card 2649 104th Street
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Dwelling | Cape Cod Style | Shore Acres (Toledo, Ohio) | Point Place (Toledo, Ohio) | North Toledo Area (Toledo, Ohio) | 2649 104th Street (Toledo, Ohio
2MASS 1315-2649
No full textIn a previous Letter, I reported that 2MASSI J1315309-264951 is an L dwarf with strong Halpha emission. Two spectroscopic epochs appeared to show that the Halpha was variable, decreasing from 121 to 25 Angstrom EW, which I interpreted as a flare during the first observation. Gizis independently discovered this object, and his intermediate spectroscopic epoch shows Halpha with 97 Angstrom EW. A new fourth epoch of spectroscopy again shows a very large Halpha EW (124 A), confirming this object to be a persistent, strong Halpha emitter. Whether the Halpha is steady (like 2MASS 1237+6526) or the result of continuous strong flaring (like PC 0025+0447) remains unclear. Imaging confirms that 2MASS 1315-2649 has a high proper motion (0."71 yr(-1)), corresponding to a transverse velocity of similar to76 km s(-1) at its distance of similar to23 pc. Thus, 2MASS 1315-2649 is consistent with being greater than or similar to2 Gyr old and therefore relatively massive. If that is so, the correlation of Halpha activity with mass found by Gizis et al. would seem to support the continuous strong flaring scenario, although it does not rule out a brown dwarf binary accretion scenario
The radioactive Substances (Lead) Exemption Order 1962
No full textERAF: A6.SI.1962.2649STATUTORY INSTRUMENTS 1962 No. 2649 ATOMIC ENERGY AND RADIOACTIVE SUBSTANCES The Radioactive Substances (Lead) Exemption Order 196
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