Lupus molecular clouds

E459017

The Lupus molecular clouds are a nearby complex of dark interstellar clouds and star-forming regions in the constellation Lupus, notable for hosting young, low-mass stars and protostars.

All labels observed (1)

Label Occurrences
Lupus molecular clouds canonical 1

How this entity was disambiguated

Statements (44)

Predicate Object
instanceOf dark cloud complex ⓘ
molecular cloud complex ⓘ
star-forming region ⓘ
associatedWith Sco-Cen OB association ⓘ
composedPrimarilyOf molecular hydrogen ⓘ
contains Class I protostars ⓘ
Class II young stellar objects ⓘ
Class III young stellar objects ⓘ
Lupus I cloud ⓘ
Lupus II cloud ⓘ
Lupus III cloud ⓘ
Lupus IV cloud ⓘ
Lupus V cloud ⓘ
Lupus VI cloud ⓘ
Lupus VII cloud ⓘ
Lupus VIII cloud ⓘ
protoplanetary disks around young stars ⓘ
young stellar objects ⓘ
containsMolecule carbon monoxide ⓘ
dust grains ⓘ
distanceFromEarth approximately 150–200 parsecs ⓘ
approximately 500–650 light-years ⓘ
hasAgeDistribution few million years for young stellar population ⓘ
hasAlternativeName Lupus dark cloud complex ⓘ
linked to: Lupus
hasProperty low to intermediate total mass ⓘ
nearby to the Sun compared to many star-forming regions ⓘ
relatively low star-formation rate ⓘ
hasStarFormation T Tauri stars ⓘ
low-mass stars ⓘ
pre-main-sequence stars ⓘ
protostars ⓘ
locatedIn Gould Belt ⓘ
locatedInConstellation Lupus ⓘ
observedBy Atacama Large Millimeter/submillimeter Array ⓘ
Herschel Space Observatory ⓘ
Spitzer Space Telescope ⓘ
observedInWavelength infrared ⓘ
millimeter ⓘ
optical ⓘ
partOf Milky Way ⓘ
skyPosition near the Scorpius–Centaurus OB association ⓘ
usedForStudyOf early stellar evolution ⓘ
low-mass star formation ⓘ
protoplanetary disks ⓘ

How these facts were elicited

Referenced by (1)

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

Gould Belt → contains → Lupus molecular clouds ⓘ