Abstract
ABSTRACT A spectrum synthesis analysis of eight spectra obtained during the non-flaring state of the cool dMe4 flare star AD Leo, yielded a mild, consistent underabundance, about 0.4 dex with respect to the Sun, for all metals. The turbulence and rotational velocities were consistent with previous studies. If the abundance results are real, the star may be older than commonly thought, however filling in one of the line cores by emission cannot be ruled out.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Publications of the Astronomical Society of the Pacific
Paper Title
Journal
Date
