Recombination line intensities for hydrogenic ions: The fine-structure components of H I and He Ii

Details Recombination line intensities for hydrogenic ions: The fine-structure components of H I and He Ii Recombination line intensities for hydrogenic ions: The fine-structure components of H I and He Ii

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26as..135..359c&link_type=abstract

Astronomy and Astrophysics Supplement, v.135, p.359-370

Astronomy and Astrophysics

Astrophysics

16

Atomic Data, Line: Formation, Line: Profiles, \Ion{H}{Ii} Regions, Planetary Nebulae: General

Scientific paper

Emissivities have been calculated for fine-structure components of selected UV and optical recombination lines of H I and He Ii. Results are given for a range of electron temperatures and densities, and in Cases A and B of te[Baker & Menzel (1938]{baker}). Relative intensities, wavelengths and velocity shifts of the fine-structure components are tabulated. Applications to the spectra of gaseous nebulae are discussed. Depending on the temperature, density and Case, the centres of unresolved lines can shift by up to 0.9 km s(-1) for H I and 3.3 km s(-1) for He Ii. A new calibration of the Hα -[N Ii] method for determining electron temperatures is given. All tables are also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

Affiliated with

Also associated with

No associations

Rating

Recombination line intensities for hydrogenic ions: The fine-structure components of H I and He Ii does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Recombination line intensities for hydrogenic ions: The fine-structure components of H I and He Ii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Recombination line intensities for hydrogenic ions: The fine-structure components of H I and He Ii will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1442627