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Table · dataset · 2022

NGC 1193 and NGC 1798 CCD UBV photometry

Listed in IVOA Registry (Virtual Observatory)

We present photometric, astrometric, and kinematic studies of the old open star clusters NGC 1193 and NGC 1798.

Description

Both of the clusters are investigated by combining data sets from Gaia Early Data Release 3 (EDR3) and CCD UBV observational data. E(B-V) color excesses are derived for NGC 1193 as 0.150(0.037) and for NGC 1798 as 0.505(0.100)mag through the use of two-color diagrams.

Photometric metallicities are also determined from two-color diagrams with the results of [Fe/H]=-0.30(0.06)dex for NGC 1193 and [Fe/H]=-0.20(0.07)dex for NGC 1798. The isochrone fitting distance and age of NGC 1193 are 5562(381) pc and 4.6(1)Gyr, respectively. For NGC 1798, these parameters are 4451(728)pc and 1.3(0.2)Gyr.

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Kinematic and dynamic orbital calculations indicate that NGC 1193 and NGC 1798 belong to the thick-disk and thin-disk populations, respectively.

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Stated by source
Optical
Provenance · 1 source records, 8 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/other/rmxaa/58.33314 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0