Coronal effects of the winds of early-type stars

Details Coronal effects of the winds of early-type stars Coronal effects of the winds of early-type stars

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..215w&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 215-218 (SEE N85-20961 1

Astronomy and Astrophysics

Astronomy

Early Stars, Hot Stars, Stellar Coronas, Stellar Winds, Ultraviolet Spectra, X Rays, Carbon, Ionization, Iue, Line Spectra, Nitrogen, Radiation Absorption, Silicon, Velocity

Scientific paper

The X-ray emission fom early-type stars can be a dominant factor in determining the ionization structure of a stellar wind. Using a base coronal model, the UV resonance lines of N V, Si IV, and C IV are calculated by subjecting them to changes in the coronal emission measure, coronal temperature, and mass loss rate. The calculations predict that a unique behavior is present in the variations of these line profiles. This suggests that it would be possible to distinguish which quantity was responsible for the variation. A preliminary search for this predicted variability, using the high-resolution short wave prime (SWP) data from the IUE archives, was conducted for several stars.

Affiliated with

Also associated with

No associations

Rating

Coronal effects of the winds of early-type 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 Coronal effects of the winds of early-type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coronal effects of the winds of early-type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-738392