Catalog Service: Stroemgren photometry of NGC 6192 and NGC 6451
Description
We have investigated the two open clusters NGC 6192 and NGC 6451 for which widely different reddening values and thus ages and distances via Stroemgren uvby photometry can be found in the literature. Our measurements allow us to disentangle the apparent discrepancies in the literature and to derive new accurate values. From appropriate calibrations we find that the overall abundance for NGC 6192 is about solar whereas a subsolar value for NGC 6451 was estimated. From two previous reported photometrically candidate CP stars, one within NGC 6192 shows Stroemgren indices typical for a B8Si star whereas the other object of NGC 6451 is most probably a foreground G-type star.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2003 Sep 16 06:44:49ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
Cone search capability for table J/A+A/403/937/table3 (Observed program stars of NGC 6192)
VERB=1
VERB=3
Cone search capability for table J/A+A/403/937/stars (NGC 6192 star positions (from Simbad), for stars with WEBDA number)
Cone search capability for table J/A+A/403/937/table4 (Observed program stars of NGC 6451)
Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
This NAVO Application is hosted by the Space Telescope Science Institute