A NEW METHOD FOR CLASSIFYING FLARES OF UV Ceti TYPE STARS: DIFFERENCES BETWEEN SLOW AND FAST FLARES-Reference-Cited by-同舟云学术

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A NEW METHOD FOR CLASSIFYING FLARES OF UV Ceti TYPE STARS: DIFFERENCES BETWEEN SLOW AND FAST FLARES

Published:2010-07-01 Issue:2 Volume:140 Page:483-489
ISSN:0004-6256
Container-title:The Astronomical Journal
language:
Short-container-title:The Astronomical Journal

Author:

Dal H. A.,Evren S.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference43 articles.

1. Physical Processes in Magnetically Driven Flares on the Sun, Stars, and Young Stellar Objects

2. Analysis and modeling of high temporal resolution spectroscopic observations of flares on AD Leonis

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