Spectrophotometry of V711 Tauri

Details Spectrophotometry of V711 Tauri Spectrophotometry of V711 Tauri

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.152...85j&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 152, no. 1, Feb. 1989, p. 85-88.

Astronomy and Astrophysics

Astrophysics

2

Binary Stars, Stellar Luminosity, Stellar Spectrophotometry, Stellar Magnitude, Tables (Data), Taurus Constellation, Visible Spectrum

Scientific paper

Spectrophotometric observations of the RS CVn binary system V711 Tau (HR 1099) have been obtained in the 3300-7100-A wavelength region. The standard spectral scans of V711 have been compared with scans of stars of known spectral types and luminosity classes taken from the Breger (1976) catalog, revealing that, at all phases shown in the diagram, the spectral-luminosity type of the star is K0IV or K0III. The system magnitude is found to fluctuate between 5.71 and 5.79 mag (with the faintest being near 0.43 p and the brightest near 0.78 p) and to average about 5.75 mag. The results show variability in the region around the Balmer jump and near the H-alpha region.

Affiliated with

Also associated with

No associations

Rating

Spectrophotometry of V711 Tauri 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 Spectrophotometry of V711 Tauri, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrophotometry of V711 Tauri will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1884219