Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...288..310b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 288, Jan. 1, 1985, p. 310-328.
Astronomy and Astrophysics
Astrophysics
19
Chromosphere, Giant Stars, Late Stars, Stellar Rotation, Ultraviolet Spectra, Emission Spectra, H Lines, Iue, K Lines, Magnesium, Periodic Variations
Scientific paper
Archival data from the International Ultraviolet Explorer have been used to study temporal variations of the Mg II h and k emission lines in eight late-type giants. Evidence is presented that the variations are periodic in nature. It is argued that the periodicities can be interpreted in terms of rotation. It is found that the four fastest rotators in the sample are 'hybrid' stars.
Brosius Jeffrey W.
Mullan Dermott J.
Stencel Robert E.
No associations
LandOfFree
Rotational modulation of chromospheric emission in cool giants and 'hybrid' 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 Rotational modulation of chromospheric emission in cool giants and 'hybrid' stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rotational modulation of chromospheric emission in cool giants and 'hybrid' stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-925287