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Table · dataset · 2024

Cataclysmic variable orb. periods from Gaia phot.

Listed in IVOA Registry (Virtual Observatory)

The orbital-period (Porb) gap in the population of cataclysmic variables (CVs) informs the theoretical narrative of CV evolution, yet a complete understanding of the driving angular momentum loss mechanisms above and below this gap remains elusive.

Description

Here we identify, for standard CVs, a new, apparently monotonic relationship between quiescent color (G_BP_-G_RP_), absolute magnitude (M_G_), and Porb (between 70 minutes and 8hr) revealed in Gaia DR2 and EDR3.

We show that Porb increases in the color-absolute-magnitude diagram roughly orthogonally to the white dwarf and main sequences. We find the orbital-period-color-absolute-magnitude relationship to be stable across different CV subtypes: dwarf novae, intermediate polars, polars, and novalike systems. We place our findings in context with the known semiempirical donor sequence for CVs and find a dependence between color and MG for a given Porb specifically for dwarf novae and intermediate polars above the period gap.

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These relations have the potential to inform a more complete picture of CV evolution.

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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/apj/938/4614 d agoJSON v1
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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