The effects of the velocity stratification of a Mira photosphere on line strengths and curves of growth

Details The effects of the velocity stratification of a Mira photosphere on line strengths and curves of growth The effects of the velocity stratification of a Mira photosphere on line strengths and curves of growth

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...253..203s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 253, no. 1, Jan. 1992, p. 203-209.

Astronomy and Astrophysics

Astrophysics

15

Abundance, Late Stars, Mira Variables, Photosphere, Stellar Spectra, Turbulent Flow, Dynamic Models, Flow Velocity, Line Spectra, Shock Fronts, Spectrum Analysis, Static Models, Stellar Models

Scientific paper

Microturbulent-broadening misinterpretation of the velocity stratification of a Mira photosphere due to matter-outflow below, and matter-infall above, the outgoing shock front, leads to incorrect results. It is presently noted that the strengths of weak lines and blue-shifted lines with symmetric profiles formed below the shock front, since they do not strictly depend on outflow/infall velocities, can be subjected to classical coarse analysis.

Affiliated with

Also associated with

No associations

Rating

The effects of the velocity stratification of a Mira photosphere on line strengths and curves of growth 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 The effects of the velocity stratification of a Mira photosphere on line strengths and curves of growth, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The effects of the velocity stratification of a Mira photosphere on line strengths and curves of growth will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-933477