Infrared photometry of the RS CVn binary HR 1099 /V711 Tau/

Details Infrared photometry of the RS CVn binary HR 1099 /V711 Tau/ Infrared photometry of the RS CVn binary HR 1099 /V711 Tau/

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..67..469a&link_type=abstract

Astrophysics and Space Science, vol. 67, no. 2, Feb. 1980, p. 469-476.

Astronomy and Astrophysics

Astronomy

9

Astronomical Photometry, Astronomical Spectroscopy, Binary Stars, Infrared Astronomy, Infrared Photometry, Phase Shift, Stellar Magnitude, Stellar Temperature

Scientific paper

Infrared observations in J, H and K of the RS CVn-type binary HR 1099 (V711 Tau) show apparent light variations similar to those in the visible. The phase shift towards increasing phase is confirmed. There is no conspicuous infrared excess attributable to circumstellar emission. The amplitudes of the infrared variation are compatible with the spot model proposed for RS CVn and enable plausible limits on a characteristic spot temperature and effective spot area to the set.

Affiliated with

Also associated with

No associations

Rating

Infrared photometry of the RS CVn binary HR 1099 /V711 Tau/ 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 Infrared photometry of the RS CVn binary HR 1099 /V711 Tau/, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infrared photometry of the RS CVn binary HR 1099 /V711 Tau/ will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1620454