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Setches, K N, 5926
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/416139Surname: SETCHES. Given Name(s) or Initials: K N. Military Service Number or Last Known Location: 5926. Missing, Wounded and Prisoner of War Enquiry Card Index Number: 16478.238292
Item: [2016.0049.48400] "Setches, K N, 5926
Block Card 5926 Carpenter Drive
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: Shotgun houses | 5926 Carpenter Drive (Toledo, Ohio) | Dwelling | Oak Grove Gardens (Toledo, Ohio) | Reynolds Corners Area (Toledo, Ohio
Block Card 5926 Hill 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: Bungalow Style | 5926 Hill Avenue (Toledo, Ohio) | Dwelling | Oak Grove Gardens (Toledo, Ohio) | Reynolds Corners Area (Toledo, Ohio) | Gable front house
Is CGCS 5926 a symbiotic X-ray binary?
No full textWe report on multiwavelength (X-ray to optical) follow-up observations of the carbon star CGCS 5926. These were motivated by the fact that this star is positionally coincident with a faint X-ray emitting object belonging to the ROSAT catalog of sources, thus suggesting a possible symbiotic X-ray binary (SyXB) nature for it. Our spectrophotometric optical data confirm the giant carbon star nature of the object and allow us to classify its spectral type as C(6,2). This classification places CGCS 5926 at a distance of ~5 kpc from Earth. BVRCIC photometry of the star shows that it displays a variability of ~0.3 mag on timescales of months, with the star getting bluer when its brightness increases. Our photometric data indicate a periodicity of 151 days, which we explain as due to radial pulsations of CGCS 5926 on the basis of its global characteristics. The source is not detected at X-rays with Swift/XRT down to a 0.3−10 keV band luminosity of ≈3 × 1032 erg s-1. This nondetection is apparently in contrast with the ROSAT data; however we show that, even if the probability that CGCS 5926 can be a SyXB appears quite low, the present information does not completely rule out such a possibility, while it makes other interpretations even more unlikely if we assume that the ROSAT detection was real. This issue might thus be settled by future, more sensitive, observations at high energies
Block Card 5926 East Heights Drive
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 | Whitmer Heights Addition (Toledo, Ohio) | Trilby Area (Toledo, Ohio)) | 5926 East Heights Drive (Toledo, Ohio
On the Symbiotic X-Ray Binary Nature of the Star CGCS 5926
No full textAbstractWe report on multiwavelength (from X-ray to optical) follow up observations of a carbon star CGCS 5926, motivated by the fact that it is positionally coincident with a faint X-ray source of the ROSAT catalog, thus suggesting its possible symbiotic X-ray binary (SyXB) nature. Our optical spectroscopy confirms that this is a carbon star of type C(6,2). This allows us to infer for CGCS 5926 a distance of ~5 kpc. BVR</jats:p
On the Symbiotic X-Ray Binary Nature of the Star CGCS 5926
No full textWe report on multiwavelength (from X-ray to optical) follow up observations of a carbon star CGCS 5926, motivated by the fact that it is positionally coincident with a faint X-ray source of the ROSAT catalog, thus suggesting its possible symbiotic X-ray binary (SyXB) nature. Our optical spectroscopy confirms that this is a carbon star of type C(6,2). This allows us to infer for CGCS 5926 a distance of ~5 kpc. BVRCIC photometry of the star shows variability of ~0.3 mag with a periodicity of 151 days, which we interpret as due to radial pulsations. the source is not detected with the Swift satellite in X-rays down to a 0.3-10 keV luminosity of ~3 × 1032 erg s−1. This nondetection is apparently in contrast with the ROSAT data; however, the present information does not rule out that CGCS 5926 can be a SyXB. This will be settled by more sensitive observations at high energies
Aerial Survey Photograph Showing Great Lakes Exhibition Site. 5926
No full textAerial Survey Photograph showing Great Lakes Exhibition Site. Surface abrasions with missing emulsion on image, scratches, marks. Dirt on top left on back of photo. Inked on top right corner of photograph "F-448". In white across bottom: 5926. Aerial Surveys, Inc."Great Lakes Exposition of 1936 and 193
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