Hyper ionization phenomena in the C IV region of 20 Oe stars

Details Hyper ionization phenomena in the C IV region of 20 Oe stars Hyper ionization phenomena in the C IV region of 20 Oe stars

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007uasb.conf..143a&link_type=abstract

UV Astronomy: Stars from Birth to Death. Proceedings of the Joint Discussion n.4 during the IAU general Assembly of 2006. Ana I.

Astronomy and Astrophysics

Astronomy

Oe Stars, Dacs, Sacs, Rotational Velocity, Gaussian Contribution, Random Velocities.

Scientific paper

Spectral lines of Oe and Be stars present DACs or SACs. In this paper we study the C IV line profiles of a sample of 20 Oe stars (from O4 to O7 spectral subtype). Using the model given by Danezis et al. (2003, 2005a,b) we found that the line shapes are very complex and that they can be fitted by a multi-component C IV region. In the sample the region may be divided into two to five subregions which show different kinematical and physical parameters. We give the kinematical parameters of subregions where the C IV resonance lines (λλ 1548.155, 1550.774 °A) are formed.

Affiliated with

Also associated with

No associations

Rating

Hyper ionization phenomena in the C IV region of 20 Oe stars 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 Hyper ionization phenomena in the C IV region of 20 Oe stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hyper ionization phenomena in the C IV region of 20 Oe stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1778069