Milky Way open cluster system

E459051

The Milky Way open cluster system is the collective population of loosely bound star clusters within our galaxy, formed from the galactic disk’s molecular clouds and serving as key tracers of its structure, star formation history, and chemical evolution.

All labels observed (1)

Label Occurrences
Milky Way open cluster system canonical 1

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf astronomical system ⓘ
population of star clusters ⓘ
affectedBy Galactic tidal field ⓘ
encounters with giant molecular clouds ⓘ
spiral arm passages ⓘ
composedOf loosely bound star clusters ⓘ
open star clusters ⓘ
containsOldPopulations yes ⓘ
containsYoungPopulations yes ⓘ
contrastsWith Milky Way globular cluster system ⓘ
hasClusterMembershipRange tens of stars to several thousand stars per cluster ⓘ
hasDynamicalState loosely gravitationally bound ⓘ
hasKinematicTracers proper motions of member stars ⓘ
radial velocities of member stars ⓘ
hasSelectionEffects incompleteness at large distances ⓘ
strong extinction near the Galactic plane ⓘ
hasSubpopulation classical open clusters ⓘ
dissolving or remnant clusters ⓘ
embedded clusters ⓘ
hasTypicalAgeRange a few million years to several billion years ⓘ
hasTypicalLifetime hundreds of millions of years for most clusters ⓘ
hasTypicalLocation Galactic thin disk ⓘ
near the Galactic plane ⓘ
hasTypicalMetallicity near-solar or supersolar metallicity ⓘ
helpsConstrain disk heating and dynamical evolution ⓘ
pattern speed of the Milky Way spiral arms ⓘ
star formation rate in the Galactic disk ⓘ
includesNotableMembers Hyades open cluster ⓘ
linked to: Hyades

Pleiades open cluster ⓘ
Praesepe open cluster ⓘ
linked to: Praesepe
locatedIn Milky Way disk ⓘ
linked to: Milky Way
observedUsing astrometric surveys such as Gaia ⓘ
infrared photometry ⓘ
optical photometry ⓘ
originatesFrom molecular clouds in the Galactic disk ⓘ
partOf Milky Way ⓘ
studiedIn Galactic disk population studies ⓘ
open cluster catalogues and surveys ⓘ
subjectOf Galactic archaeology studies ⓘ
traces Galactic chemical evolution ⓘ
Galactic disk structure ⓘ
Galactic star formation history ⓘ
Milky Way spiral arms ⓘ
usedFor calibrating the cosmic distance scale ⓘ
determining the Galactic radial metallicity gradient ⓘ
mapping the Milky Way spiral pattern ⓘ
studying stellar evolution ⓘ

How these facts were elicited

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

Open cluster M11 → partOf → Milky Way open cluster system ⓘ