SII

E491339

SII (singly ionized sulfur) is an emission line commonly used in astrophotography and spectroscopy to highlight ionized gas regions in nebulae and other astronomical objects.

All labels observed (1)

Label Occurrences
SII canonical 1

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf emission line ⓘ
ion ⓘ
singly ionized atom ⓘ
spectral line ⓘ
belongsToSpectralRegion optical ⓘ
red ⓘ
category astrophysical emission line ⓘ
nebular line ⓘ
comparedWith Hα emission ⓘ
[O III] emission ⓘ
diagnosticFor electron density in nebulae ⓘ
photoionized gas ⓘ
shock-excited gas ⓘ
emittedBy ionized interstellar medium ⓘ
photoionized nebulae ⓘ
shock fronts in supernova remnants ⓘ
hasApplication probing physical conditions in nebulae ⓘ
separating shock-ionized from photoionized regions ⓘ
studying star-forming regions ⓘ
hasAtomicNumberOfElement 16 ⓘ
hasCharge +1 ⓘ
hasChemicalSymbol S ⓘ
hasCommonWavelength 6716 Å ⓘ
6731 Å ⓘ
hasElement sulfur ⓘ
hasIonizationPotentialOfParentToThisState 10.36 eV ⓘ
hasIonizationState singly ionized ⓘ
hasSpectroscopicNotation S II ⓘ
hasTransitionType forbidden line ⓘ
mappedToColor red in Hubble palette ⓘ
observedIn active star-forming galaxies ⓘ
extragalactic H II regions ⓘ
galactic nebulae ⓘ
relatedTo interstellar medium diagnostics ⓘ
sulfur abundance measurements ⓘ
traces ionized gas ⓘ
nebular gas ⓘ
usedIn astronomical spectroscopy ⓘ
astrophotography ⓘ
usedInColorMappingScheme Hubble palette ⓘ
usedInImagingFilter S II narrowband filter ⓘ
usedInImagingTechnique narrowband imaging ⓘ
usedToHighlight H II regions ⓘ
ionized gas regions ⓘ
nebulae ⓘ
planetary nebulae ⓘ
supernova remnants ⓘ

How these facts were elicited

Referenced by (1)

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