Properties (57)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
astronomical object
|
| gptkbp:associatedWith |
star formation
|
| gptkbp:canEstablish |
variability
complex morphologies |
| gptkbp:canLeadTo |
stellar evolution
|
| gptkbp:characterizedBy |
jets of gas
|
| gptkbp:established |
gptkb:George_Herbig
Guido Haro |
| gptkbp:exhibits |
spectral lines
shock_waves |
| https://www.w3.org/2000/01/rdf-schema#label |
Herbig–Haro objects
|
| gptkbp:is_used_in |
young stars
|
| gptkbp:isCitedIn |
the context of molecular astrophysics
the context of star formation theory |
| gptkbp:isCounteredBy |
collisions of stellar jets
their bright emission lines |
| gptkbp:isCriticizedFor |
spectroscopy
imaging techniques |
| gptkbp:isFoundIn |
various galaxies
regions of high stellar density |
| gptkbp:isImportantFor |
understanding star formation
understanding cosmic evolution understanding galactic dynamics |
| gptkbp:isLocatedIn |
molecular clouds
star clusters |
| gptkbp:isOftenMadeWith |
T Tauri stars
bipolar outflows protoplanetary disks massive star formation regions |
| gptkbp:isPartOf |
star-forming regions
|
| gptkbp:isRelatedTo |
molecular outflows
|
| gptkbp:isStudiedIn |
astrophysics
numerical simulations |
| gptkbp:isUsedBy |
the interaction of stellar winds
|
| gptkbp:isUsedFor |
interstellar medium
optical wavelengths radio wavelengths the formation of planetary systems the HH 1-2 region the HH 34 region the HH 46/47 region the NGC 1333 region the Perseus molecular cloud the Rho Ophiuchi cloud infrared_wavelengths the_Carina_Nebula the_L1630_region the_Orion_Nebula the_Serpens_cloud |
| gptkbp:isUtilizedFor |
the dynamics of star formation.
the properties of young stars |
| gptkbp:isUtilizedIn |
H-alpha emission
forbidden lines |
| gptkbp:locatedIn |
nebulae
|
| gptkbp:mayHave |
stellar outflows
|
| gptkbp:stadium |
gptkb:George_Herbig
Guido Haro |