Catalog Service: H{alpha} rotation curves for 10 spiral galaxies
Description
H{alpha} rotation curves for a sample of 10 late-type spiral galaxies. All rotation curves were derived using Harmonic decomposition method applied to Fabry-Perot velocity fields. We have used the rotation curves combined with pattern speeds from the Tremaine-Weinberg method, to study the dynamics of bars and spiral arms in late-type spiral galaxies.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2009 Dec 27 19:41:52ZThis 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/ApJ/704/1657/galaxies (List of galaxies studied)
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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