Abundance analysis of the BY Draconis variable, hot flare star V833 Tauri

Details Abundance analysis of the BY Draconis variable, hot flare star V833 Tauri Abundance analysis of the BY Draconis variable, hot flare star V833 Tauri

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..565n&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 688, p. 565-567.

Astronomy and Astrophysics

Astronomy

5

Abundance, Hot Stars, Stellar Flares, Stellar Spectra, Variable Stars, Dwarf Stars, Lithium, Stellar Rotation

Scientific paper

Eight spectra of the hot flare star, V833 Tauri, K5 Ve, covering the region from 3881 to 8520 A were analyzed using a spectrum synthesis technique. The rapid rotation reported by Vogt et al. (1983) was confirmed. The abundances were essentially solar in all cases. No excess lithium abundance was seen, consistent with a possible membership in the Hyades cluster.

Affiliated with

Also associated with

No associations

Rating

Abundance analysis of the BY Draconis variable, hot flare star V833 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 Abundance analysis of the BY Draconis variable, hot flare star V833 Tauri, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Abundance analysis of the BY Draconis variable, hot flare star V833 Tauri will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1335948