Relation between the (V-R) and (R-I) color indices and activity for solar-type stars

Details Relation between the (V-R) and (R-I) color indices and activity for solar-type stars Relation between the (V-R) and (R-I) color indices and activity for solar-type stars

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99..288r&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, April 1987, p. 288-296.

Other

7

Late Stars, Stellar Activity, Stellar Color, Stellar Spectra, Calcium, Dwarf Stars, Magnesium, Near Infrared Radiation, Subgiant Stars

Scientific paper

Bright moderately active stars with known Ca II or Mg II emission fluxes and with measured (V-R) and (R-I) color indices in the Cousins system have been checked for the presence of activity-related near-infrared excesses. With increased levels of activity, both colors show very weakly indicated excesses for subgiants and deficits for dwarfs. While the effect observed for subgiants may be related to large near-infrared excesses observed in RS CVn-type stars or other very active stars, the spectral distributions for dwarfs do not show any abnormality beyond what would be expected from the blanketing in (B-V), which was used as the reference color.

Affiliated with

Also associated with

No associations

Rating

Relation between the (V-R) and (R-I) color indices and activity for solar-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 Relation between the (V-R) and (R-I) color indices and activity for solar-type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relation between the (V-R) and (R-I) color indices and activity for solar-type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1349543