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Radiative lifetimes branching ratios, and absolute transition probabilities in Cr II and Zn II

Author
BERGESON, S. D; LAWLER, J. E
Univ. Wisconsin-Madison, dep. physics, Madison WI 53706, United States
Source

The Astrophysical journal. 1993, Vol 408, Num 1, pp 382-388 ; 1 ; ref : 43 ref

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Chrome ion Durée vie moyenne Etude en laboratoire Probabilité transition Processus atomique Rapport branchement Zinc ion Matière interstellaire
Keyword (en)
Chromium ions Lifetime Laboratory study Transition probabilities Atomic process Branching ratio Zinc ions Interstellar matter
Keyword (es)
Estudio en laboratorio Proceso atómico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A30 Fundamental aspects of astrophysics / 001E03A30D Atomic processes and interactions

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A30 Fundamental aspects of astrophysics / 001E03A30K Atomic and molecular data, spectra, and spectral parameters (opacities, rotation constants, line identification, oscillator strengths, gf values, transition probabilities, etc.)

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
3841330

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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