1,725,877 research outputs found
Block Card 3543 Hoiles Avenue
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 (Toledo, Ohio) | Side gabled | Box bay windows | Craftsman Style | West Toledo (Toledo, Ohio) | Homewood Park (Toledo, Ohio) | Willys Park area (Toledo, Ohio) | Folk House Style | 3543 Hoiles Avenue (Toledo, Ohio
Block Card 3543 Hazelhurst Avenue
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 (Toledo, Ohio) | Folk House Style | Homewood Park Extension (Toledo, Ohio) | Willys Park area (Toledo, Ohio) | West Toledo (Toledo, Ohio) | 3543 Hazelhurst Avenue (Toledo, Ohio
AGC 226178 and NGVS 3543: Two Deceptive Dwarfs toward Virgo
Get PDFThe two sources AGC 226178 and NGVS 3543, an extremely faint, clumpy, blue stellar system and a low surface brightness dwarf spheroidal, are adjacent systems in the direction of the Virgo cluster. Both have been studied in detail previously, with it being suggested that they are unrelated normal dwarf galaxies or that NGVS 3543 recently lost its gas through ram pressure stripping and AGC 226178 formed from this stripped gas. However, with Hubble Space Telescope Advanced Camera for Surveys imaging, we demonstrate that the stellar population of NGVS 3543 is inconsistent with being at the distance of the Virgo cluster and that it is likely a foreground object at approximately 10 Mpc, whereas the stellar population of AGC 226178 is consistent with it being a very young (10-100 Myr) object in the Virgo cluster. Through a reanalysis of the original ALFALFA H i detection, we show that AGC 226178 likely formed from gas stripped from the nearby dwarf galaxy VCC 2034, a hypothesis strengthened by the high metallicity measured with MUSE VLT observations. However, it is unclear whether ram pressure or a tidal interaction is responsible for stripping the gas. Object AGC 226178 is one of at least five similar objects now known toward Virgo. These objects are all young and unlikely to remain visible for over ∼500 Myr, suggesting that they are continually produced in the cluster. © 2022. The Author(s). Published by the American Astronomical Society.Open access journalThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at [email protected]
[Veto of H. 3543, R-249]
No full textThis veto message from Governor Mark Sanford vetoes H. 3543, R-249, a bill that increases the time a person who holds a license issued by the Environmental
Certification Board has to renew a lapsed license without penalty from 90 days to 365 days
3543. Chronique de Pierre IV le Cérémonieux, roi d'Aragon
No full text3543. Chronique de Pierre IV le Cérémonieux, roi d'Aragon. In: Molinier Auguste. Les Sources de l'histoire de France - Des origines aux guerres d'Italie (1494). IV. Les Valois, 1328-1461. Paris : A. Picard et fils, 1904. pp. 108-109
Morgan, Eldon Stephenson, 1879-1961 (SC 3543)
Get PDFFinding aid and scan (Click on Additional Files below) for Manuscripts Small Collection 3543. Letter, 15 September 1930, from Eldon S. Morgan, Scottsville, Kentucky Chief of Police, to Harry G. Smith, Secretary of the Kentucky Bankers Association, Louisville, Kentucky. He advises of his participation in the recent capture of a bank robber and asks for details regarding the offer and payment of a reward
Genome sequence of Lactobacillus fructivorans KCTC 3543
No full textLactobacillus fructivorans is important in the generation of particular flavors and in other ripening processes associated with fermented food. Here, we present the draft genome sequence of the type strain Lactobacillus fructivorans KCTC 3543 (1,373,326 bp, with a G+C content of 38.9%), which consists of 5 scaffolds. The genome sequence was obtained by using a whole-genome shotgun strategy with Roche 454 GS (FLX Titanium) pyrosequencing, and all of the reads were assembled using Newbler Assembler 2.3.open
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