Chromospheric activity of 9 Aurigae
2013 ◽
Vol 9
(S301)
◽
pp. 439-440
Keyword(s):
AbstractThe definition of γ Dor stars as a new class of variable stars by Kaye et al. (1999) was based on a number of criteria, including the failure to detect any emission in the Ca II H & K lines in these stars (Kaye & Strassmeier 1998; KS98). Over the last 30 years, efforts continue to look for the blue edge of chromospheric activity. As a part of this effort, we put γ Dor stars to the test to see if magnetic fields play a non-trivial role in their variability.
2021 ◽
Vol 14
(1)
◽
Keyword(s):
2019 ◽
Vol 1
(1)
◽
pp. 3411-3420
1992 ◽
Vol 439
(1907)
◽
pp. 441-463
◽
Keyword(s):
2003 ◽
Vol 35
(02)
◽
pp. 319-336
◽
Keyword(s):
Keyword(s):
2005 ◽
Vol 1
(T26A)
◽
pp. 245-245