Alpha² Canum Venaticorum variable
Let an agent describe alpha2 CVn variables by star, period, magnetic field and spectroscopy, with sourced data.
Bundle → Layer → Finding → Questions Filled
4 bundles · 8 layers · 8 findings · 16 questions
Star Which star.
Identity
Designation.
Identity
Designation.
- Which star is meant, and is it classified as ACV? provenance
- What is its spectral type? provenance
Period
Rotation.
Period
Rotation period.
- What is its rotation period and amplitude? measurement
- From which survey data? provenance
Physics Magnetism.
Field
Magnetic field.
Field
Magnetic field.
- How strong is the magnetic field, according to spectropolarimetry? measurement
- How is it oriented? provenance
Spots
Abundance spots.
Spots
Chemical spots.
- Which elements are concentrated in surface spots? provenance
- How are spot maps made? definition
Classes Related types.
roAp
Rapid oscillators.
roAp
Rapidly oscillating Ap stars.
- Does the star also show rapid oscillations? provenance
- How do roAp stars differ from ACV variables? definition
Chemically peculiar
Ap and Bp stars.
Chemically peculiar
Chemical peculiarity.
- What makes Ap and Bp stars chemically peculiar? definition
- Which processes explain it? provenance
Observing Contributing.
Photometry
Small amplitudes.
Photometry
Photometry.
- What photometric precision is needed to detect the variation? measurement
- Can amateurs contribute? boundary
Submit
Databases.
Submit
Submitting data.
- How can observations be submitted to variable star databases? action
- Which organisation runs them? provenance
Classifiers Filled
- Family
- Thing Registry
- Category
- Physical world and living systems
- Entry kind
- thing
- Plane
- PHY
- Domain
- PHY.SPC
- Other names and narrower kinds
- rapidly oscillating Ap star
What it is Filled
A chemically peculiar Ap or Bp main-sequence star with a strong, ordered magnetic field and surface abundance spots, whose brightness and spectrum vary with rotation over periods of about 0.5 to 160 days; named after Alpha2 Canum Venaticorum. Rapidly oscillating Ap stars are a related class with pulsations of minutes.
Why it exists Filled
Let an agent describe alpha2 CVn variables by star, period, magnetic field and spectroscopy, with sourced data.
Distinguishing features Filled
- Strong magnetic fields
- Chemical spots
- Rotational variability
- Oblique rotator model
What robots and AI may and may not do Filled
Must not
- Confuse these stars with rapidly oscillating Ap stars.
- Claim a new variable star from small amplitude signals without checking for instrument effects.
- Alter catalogue entries without stating the source of the change.
Only with a human decision
- Submitting a new classification to a variable star catalogue.
May
- Report catalogued Alpha2 Canum Venaticorum variables with their periods and sources.
- Analyze light curves and spectra to classify a star as this type, stating the uncertainty.
Moral aspects Filled
- Honest reporting of weak signals keeps the astronomical record trustworthy.
Who is affected
- Astronomers and observers
- Users of variable star catalogues
Owners Filled
Steward
Nobody owns them; variable star catalogues and the astronomical community keep the records.
Master systems
- General Catalogue of Variable Stars
- International Variable Star Index
Links to other meta-models Filled
parent
- Q2168098 - registry parent class
- Q616386 - registry parent class
related
- rotating variable star and Ap/Bp star - category
- Alpha2 Canum Venaticorum - prototype
- oblique rotator model - theory
- GCVS and VSX - catalogues
What else AI and robots need to interact with it Filled
Identity and identifiers required Filled
- Vercy registry: vr.tr.alpha-canum-venaticorum-variable
- Wikidata: Q1141942 (https://www.wikidata.org/wiki/Q1141942)
- GCVS type: ACV variable star type
Direct properties required Filled
- rotation period: about 0.5-160 days
- amplitude: about 0.01-0.1 magnitudes - typical
Recognition required Filled
- Ap or Bp spectral types
- Rotation-linked variability
- roAp stars pulsate on minute timescales
- Blue-white stars with small periodic brightness changes.
Capabilities and actions required Filled
- identify alpha2 CVn stars and periods
- explain rotational modulation
- distinguish them from roAp stars
- find photometric and spectroscopic data
Hazards and failure modes required Filled
- Confusing ACV and roAp stars
- Overinterpreting small amplitudes
Standards and interfaces required Filled
- IAU variable star nomenclature
Context of use required Filled
- Studying stellar magnetism and chemical peculiarity.
- classical alpha2 CVn variables
- magnetic Bp stars
- rapidly oscillating Ap stars (related)
Sources Filled
- Wikidata item Q1141942: Alpha² Canum Venaticorum variable - identity and sense of the item
- Wikipedia: Alpha2 Canum Venaticorum variable - general description of the item
Open questions
- Should roAp stars be a separate entry?
- How should magnetic field data be linked?
- How should spot maps be sourced?
Machine files
Provenance
thing registry research (pass 2) · unreviewed
Built from: models/things/publications/thing-q1141942/spec.json