Stark profiles of infrared helium lines

Details Stark profiles of infrared helium lines Stark profiles of infrared helium lines

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..133..229t&link_type=abstract

Astronomy and Astrophysics Supplement, v.133, p.229-244

Astronomy and Astrophysics

Astrophysics

1

Stars: Early-Type, Infrared: General, Atomic Data, Lines: Profiles

Scientific paper

We have calculated Stark widths and shifts of some infrared helium lines that are missing and that are important for modellisation of the atmospheres of hot early-type stars. These calculations are based on the impact and quasistatic theory and semi-classical approximation. The provided data are displayed for a grid of temperatures ( 10(4) to 10(5) K) and electron densities (10(10) to 10(13) cm(-3) ) typical of hot early-type stars. We also discuss the conditions of use of our data for astrophysical purposes.

Affiliated with

Also associated with

No associations

Rating

Stark profiles of infrared helium lines 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 Stark profiles of infrared helium lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stark profiles of infrared helium lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-992013