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On the Use of the [Zn IV] 3.625 Micron Line as a Tracer of Iron-group Abundances in Ionized Nebulae
On the Use of the [Zn IV] 3.625 Micron Line as a Tracer of Iron-group Abundances in Ionized Nebulae
2007
Harriet L. Dinerstein
Th. R. Geballe
Jessica L. Wood
N. C. Sterling
Keywords:
Zinc
TRACER
Iron group
Planetary nebula
Atomic physics
Astronomy
Infrared
Milky Way
Emission spectrum
Emission nebula
Physics
Correction
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