Oscillator strength and linewidth measurements of dipole-allowed transitions in 14N 14 between 93.5 and 99.5 nm

Journal of Chemical Physics

Volumn 123, Issue 21, 2005, Pages

  Stark, G ^a   Huber, K P ^b   Yoshino, K ^c   Smith, Peter L ^c   Ito, K ^d  

^a WELLESLEY COLLEGE   (United States)

^b NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d HIGH ENERGY ACCELERATOR RESEARCH ORGANIZATION KEK   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

INSTRUMENTAL RESOLUTION; LINE OSCILLATOR STRENGTH; LINEWIDTH MEASUREMENTS; ROTATIONAL INTERACTIONS;

MATHEMATICAL MODELS; NONLINEAR EQUATIONS; OSCILLATORS (ELECTRONIC); POLYNOMIALS; SPECTROSCOPIC ANALYSIS;

OPTICAL RESOLVING POWER;

EID: 28944434495     PISSN: 00219606     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.2134703     Document Type: Article

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63. The plate was recorded on the 6.65 m vacuum spectrometer at the Harvard-Smithsonian Center for Astrophysics with a helium continuum light source [K. Yoshino (unpublished)].