Catalog Service: Multiwavelength study of NGC 7419
Description
Using new UBVRI H{alpha} CCD photometric observations and the archival infrared and X-ray data, we have carried out a multiwavelength study of a Perseus arm young open star cluster NGC 7419. Using XMM-Newton observations, we found several X-ray sources in the cluster region but none of the Herbig Ae/Be stars is detected in X-rays.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2009 Jun 27 22:15:10ZThis 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/MNRAS/391/1279/table3 (UBVRI and H{alpha} photometric data of the sample stars in 13'x13' region)
VERB=1
VERB=3
Cone search capability for table J/MNRAS/391/1279/table6 (Photometric properties of 44 H{alpha} emission-line stars in 13x13arcmin^2^ region around NGC 7419)
Cone search capability for table J/MNRAS/391/1279/table13 (X-ray sources detected using SAS task edetect_chain)
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