Asymmetries in stellar MG II H and K and CA II H and K line profiles - Discrepancies between MG and CA asymmetries

Details Asymmetries in stellar MG II H and K and CA II H and K line profiles - Discrepancies between MG and CA asymmetries Asymmetries in stellar MG II H and K and CA II H and K line profiles - Discrepancies between MG and CA asymmetries

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...284..769m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 284, Sept. 15, 1984, p. 769-773.

Astronomy and Astrophysics

Astrophysics

14

Emission Spectra, Giant Stars, H Lines, K Lines, Late Stars, Spectral Energy Distribution, Stellar Spectra, Stellar Winds, Asymmetry, Calcium, Magnesium, Potassium, Spectral Line Width, Stellar Rotation, Ultraviolet Spectra

Scientific paper

"Discrepant asymmetry" stars are cool giants which show the opposite
sense of asymmetry in the emission cores of Ca and Mg (i.e., red peak
dominant in Mg, blue peak dominant in Ca). The author suggests that
these discrepancies can be understood in terms of corotating interaction
regions in the winds.

Affiliated with

Also associated with

No associations

Rating

Asymmetries in stellar MG II H and K and CA II H and K line profiles - Discrepancies between MG and CA asymmetries 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 Asymmetries in stellar MG II H and K and CA II H and K line profiles - Discrepancies between MG and CA asymmetries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Asymmetries in stellar MG II H and K and CA II H and K line profiles - Discrepancies between MG and CA asymmetries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1390588