Radiative lifetimes and transition probabilities in Hf I and Hf IIIShow others and affiliations
2009 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 396, no 4, p. 2289-2294Article in journal (Refereed) Published
Abstract [en]
The infrared (IR) atomic spectral lines that can be observed in laboratory and astrophysical spectra depend both on the atomic structure and the physical conditions in which the atoms reside. This is a brief review of IR laboratory spectroscopy, discussing which lines in the wavelength interval 1–5 μm can be expected to be seen in different astrophysical sources.
Place, publisher, year, edition, pages
Institute of Physics Publishing (IOPP), 2009. Vol. 396, no 4, p. 2289-2294
National Category
Atom and Molecular Physics and Optics
Identifiers
URN: urn:nbn:se:mau:diva-63266DOI: 10.1111/j.1365-2966.2009.14894.xISI: 000267710400036OAI: oai:DiVA.org:mau-63266DiVA, id: diva2:1807692
2023-10-272023-10-272023-10-27Bibliographically approved