Spectral synthesis analysis and radial velocity study of the northern F-, G-, and K-type flare-stars

Details Spectral synthesis analysis and radial velocity study of the northern F-, G-, and K-type flare-stars Spectral synthesis analysis and radial velocity study of the northern F-, G-, and K-type flare-stars

2005-11-08

arxiv.org/abs/astro-ph/0511232v1

Mon.Not.Roy.Astron.Soc.365:1050,2006

Astronomy and Astrophysics

Astrophysics

8 pages, 9 figures, accepted by MNRAS

Scientific paper

10.1111/j.1365-2966.2005.09796.x

In this publication we present a study of the general physical, chemical properties and radial velocity monitoring of young active stars. We derive temperatures, log g, [Fe/H], v sin i, and R_{spec} values for eight stars. The detailed analysis reveals that the stars are not as homogeneous in their premier physical parameters as well as in the age distribution. In 4/5 we found a periodic radial velocity signal which origins in surface features the fifth is surprisingly inactive and shows little variation.

Affiliated with

Also associated with

No associations

Rating

Spectral synthesis analysis and radial velocity study of the northern F-, G-, and K-type flare-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 Spectral synthesis analysis and radial velocity study of the northern F-, G-, and K-type flare-stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral synthesis analysis and radial velocity study of the northern F-, G-, and K-type flare-stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-293435