1,724,211 research outputs found
Baltimore & Ohio (B&O) 5236
No full textA photograph print showing Baltimore & Ohio (B&O) 5236, 4-6-2 (P-7)
La región nuclear de NGC 5236
Get PDFObservaciones mono y heterocromáticas han permitido establecer la estructura nuclear de NGC 5236.Asociación Argentina de Astronomí
Effects of Automated Static Analysis Tools: A Multidimensional View on Quality Evolution
No full textBlock Card 5236 Kellogg Road
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: Ranch houses | Dwelling | Homedale Addition (Toledo, Ohio) | Reynolds Corners Area (Toledo, Ohio) | 5236 Kellogg Road (Toledo, Ohio
Block Card 5236 Nebraska 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: Ranch houses | Dwelling | Homedale Addition (Toledo, Ohio) | Reynolds Corners Area (Toledo, Ohio) | 5236 Nebraska Avenue (Toledo, Ohio
Cerámica en el mecado, "5236. Aguascalientes. Pottery market"
No full textI.O. Anverso: "5236. Aguascalientes. Pottery market". V.F. 450140
Block Card 5236 Brandon Road
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: 5236 Brandon Road (Toledo, Ohio) | Dwelling | Extension of Homedale Addition (Toledo, Ohio) | Reynolds Corners Area (Toledo, Ohio) | Cape Cod Styl
Black Hole Ejected from the Nucleus of Galaxy NGC 5236
Get PDFThe Fanaroff-Riley II-type radiosource J 133658.3-295105, which is also an X-ray source, appears to be projected onto the disc of the barred-spiral galaxy NGC 5236 (M 83) at about 1.2 kiloparsecs from the galaxy´s optical nucleus. J 133658.3-295105, its radio-lobes, and two other radiosources, neither of which are supernovae remnants or HII regions, are aligned with the optical nucleus of NGC 5236. Due to this peculiar on-the-sky projection, we studied J 133658.3-295105 using GEMINI+GMOS optical spectroscopy and also reanalyzed Chandra spectroscopy which was carried out in 2000. We marginally detected the Hα emission line receding at 130 km/sec with respect to the optical nucleus. We also demostrate that J 133658.3-295105 presents the Fe-Kα emission line at a redshift z = 0.018 ± 0.01. Both, Hα and Fe-Kα present redshifts that are compatible with the distance of NGC 5236. That findings reinforce the scenario of a local object for J 133658.3-295105, which could have been ejected from the nucleus of NGC 5236.Fil: Dottori, H.. Universidade Federal do Rio Grande do Sul; BrasilFil: Diaz, Ruben Joaquin. Gemini Observatory; Estados Unidos. Consejo Nacional de Investigaciones CientiÂficas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; ArgentinaFil: Albacete Colombo, J. F.. Universidad Nacional del Comahue; ArgentinaFil: Mast, D.. Centro Astronómico Hispano Alemán; Españ
Cerámica en el mecado, "5236. Aguascalientes. Pottery market"
No full textI.O. Anverso: "5236. Aguascalientes. Pottery market". Reverso: "3230". Información en el título, fecha de toma y asunto, proporcionada por Nacho Gutiérrez R., diciembre de 2009. V.F. 450293
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