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