Catalog Service: H{alpha} emission objects in the southern Milky Way
Description
The stars reported in James Wray's PhD thesis result from photographic plates taken by Karl Henize in South Africa during 1949-1951 covering the Southern Galactic plane to about 10{deg} latitude. Accurate positions of the stars studied in the PhD thesis were recovered by B. Skiff, see details in the "intro.txt" file.
This section describes who is responsible for this resource
Publisher: CDSivo://CDS[Pub. ID]
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This section provides some status information: the resource version, availability, and relevant dates.
This resource was registered on: 2016 Nov 04 12:12:27ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
This section describes what the resource is, what it contains, and how it might be relevant.
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This section describes the data's coverage over the sky, frequency, and time.
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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 III/277/wray_neb (Combined table from original tables)
VERB=1
VERB=3
Cone search capability for table III/277/wray_15 (Table 15: emission stars)
Cone search capability for table III/277/wray_18 (Table 18: C- and S-type stars)
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