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Table · dataset · 2009

Velocity and H{alpha} width of 22 Vul

Listed in IVOA Registry (Virtual Observatory)

The 22 Vul system is important for studying the winds and chromospheres of cool evolved stars because the G4 I component is rotating rapidly and probably faster than synchronously.

Description

We discuss the system's physical properties in the context of a wide range of constraints on them and propose values that may be marginally better than previous ones. We use H{alpha} spectroscopy to assess the variability of the cool star's wind, and archival IUE observations to measure variation of density in the wind and rotation of the chromosphere.

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Catalogue records · 2

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Optical
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Astronomical sciences 73%
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/aj/133/266914 d agoJSON v1
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concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
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