A study of the atmospheric structure of AX Mon (HD 45910)

Details A study of the atmospheric structure of AX Mon (HD 45910) A study of the atmospheric structure of AX Mon (HD 45910)

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009coast.159..119a&link_type=abstract

"Communications in Asteroseismology, Vol. 159, p. 119-120. Proceedings of "JENAM 2008 Symposium No 4: Asteroseismology and Stell

Physics

Scientific paper

In this paper we apply the GR model to find kinematic parameters (radial, rotational and random velocities) as well as FWHM, the absorbed energy and the Gaussian Typical Deviation (σ) for a group of Fe II spectral lines from AX Mon spectra obtained with IUE. In order to find possible stratification in the Fe II absorbing region of AX Mon we present these parameters as a function of the excitation potential of the lines. We found that the obtained parameters are not too sensitive to the excitation potential of the Fe II lines. In addition, we calculate the above mentioned parameters for the Al II (λ 1670.81 Å), Al III (λ λ 1854.722, 1867.782 Å), Mg II (λ λ 2795.523, 2802.698 Å), Fe II (λ 2586.876 Å), C II (λ λ 1334.515, 1335.684 Å) and Si IV (λ λ 1393.73, 1402.73 Å) spectral lines of AX Mon, and we present their relation with the ionization potential.

Affiliated with

Also associated with

No associations

Rating

A study of the atmospheric structure of AX Mon (HD 45910) 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 A study of the atmospheric structure of AX Mon (HD 45910), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A study of the atmospheric structure of AX Mon (HD 45910) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-973435