Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..163m&link_type=abstract
Astronomical Society of the Pacific, Publications, vol. 87, Feb. 1975, p. 163-171.
Astronomy and Astrophysics
Astronomy
10
Astronomical Models, Dwarf Stars, Emission Spectra, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, Eclipses, Electrophotometry, Error Analysis, Line Spectra
Scientific paper
Photoelectric UBVRI photometry of LP101-15, BY Dra, GT Peg, and FF And is presented, and implications with respect to the 'center-of-activity' model are discussed. This is apparently the most physically acceptable model to date; facular-like areas and flare activity are included in an attempt to explain all aspects of the behavior of this class of stars. Data for BY Dra and GT Peg are inconclusive at this time, but FF And can be fairly well understood in terms of the center-of-activity model. A slight secondary eclipse may have been detected for LP101-15, but verification is needed.
No associations
LandOfFree
Observations of the red-dwarf emission-line objects LP101-15, BY Draconis, GT Pegasi, and FF Andromedae 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 Observations of the red-dwarf emission-line objects LP101-15, BY Draconis, GT Pegasi, and FF Andromedae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of the red-dwarf emission-line objects LP101-15, BY Draconis, GT Pegasi, and FF Andromedae will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1000196