The young active binary star EK Draconis
نویسندگان
چکیده
منابع مشابه
The Corona of the Young Solar Analog Ek Draconis
First coronal microwave and new soft X-ray observations (complementary to those reported by Dorren et al. 1995) of the very active, near-Zero-Age Main-Sequence (ZAMS) dG0e star EK Dra = HD 129333 show that this analog of the young Sun is more luminous in both emissions than most single M-dwarf are stars. Variations in the 8.4 GHz ux include the optically determined rotation period of 2.7 days. ...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2005
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361:20040462