Lynds 1641

E459026

Lynds 1641 is a prominent star-forming molecular cloud region within the Orion Molecular Cloud Complex, known for its young stellar objects and ongoing low- to intermediate-mass star formation.

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Statements (48)

Predicate Object
instanceOf giant molecular cloud
molecular cloud
star-forming region
cataloguedIn Lynds Dark Nebula catalog NERFINISHED
contains Class 0 protostars
Class I protostars
Class II pre-main-sequence stars
Herbig–Haro objects NERFINISHED
T Tauri stars NERFINISHED
dense cores
embedded young stellar clusters
filamentary structures
molecular outflows
distanceFromEarth approximately 1300 light-years
approximately 400 parsecs
hasAgeProperty contains very young stellar population
hasComponent L1641-C region NERFINISHED
L1641-N region NERFINISHED
L1641-S region NERFINISHED
hasDust interstellar dust
hasEnvironment less massive stars than Orion Nebula Cluster
relatively low stellar density compared to Orion Nebula Cluster
hasGas carbon monoxide
molecular hydrogen
hasProperty contains young stellar objects
obscured in optical wavelengths by dust
ongoing star formation
prominent star-forming region
hasResearchUse study of circumstellar disks
study of clustered star formation
study of low-mass star formation
study of protostellar evolution
hasStarFormationMode clustered star formation
distributed star formation
hasStarFormationType intermediate-mass star formation
low-mass star formation
isSouthOf Orion Nebula Cluster NERFINISHED
locatedIn constellation Orion NERFINISHED
observedIn infrared wavelengths
millimeter wavelengths
submillimeter wavelengths
partOf Orion A molecular cloud NERFINISHED
Orion Molecular Cloud Complex NERFINISHED
studiedBy Herschel Space Observatory NERFINISHED
Spitzer Space Telescope NERFINISHED
ground-based radio telescopes
tracedBy CO emission
dust continuum emission

Referenced by (1)

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