2014A&A...571A..74K -
Astronomy and Astrophysics, volume 571A74-74 (2014/11-1)
Lithium enrichment on the single active K1-giant DI Piscium. Possible joint origin of differential rotation and Li enrichment.
KRISKOVICS L., KOVARI Z., VIDA K., GRANZER T. and OLAH K.
Abstract (from CDS):
We investigate the surface spot activity of the rapidly rotating, lithium-rich active single K-giant DI Psc to measure the surface differential rotation and understand the mechanisms behind the Li-enrichment. Doppler imaging was applied to recover the surface temperature distribution of DI Psc in two subsequent rotational cycles using the individual mapping lines CaI 6439, FeI 6430, FeI 6421, and LiI 6708. Surface differential rotation was derived by cross-correlation of the subsequent maps. Difference maps are produced to study the uniformity of Li-enrichment on the surface. These maps are compared with the rotational modulation of the LiI 6708 line equivalent width. Doppler images obtained for the Ca and Fe mapping lines agree well and reveal strong polar spottedness, as well as cool features at lower latitudes. Cross-correlating the consecutive maps yields antisolar differential rotation with a shear coefficient α=-0.083 ±0.021. The difference of the average and the Li maps indicates that the lithium abundance is non-activity related. There is also a significant rotational modulation of the Li equivalent width.
Abstract Copyright:
∼
Journal keyword(s):
stars: activity - stars: imaging - stars: late-type - starspots - stars: individual: DI Psc
Simbad objects:
5
Full paper
View the references in ADS
To bookmark this query, right click on this link: simbad:2014A&A...571A..74K and select 'bookmark this link' or equivalent in the popup menu