Titlebook: Cool Stars, Stellar Systems, and the Sun; Proceedings of the T Sallie L. Baliunas,Lee Hartmann Conference proceedings 1984 Springer-Verlag

CHORD

书目名称Cool Stars, Stellar Systems, and the Sun影响因子(影响力)




书目名称Cool Stars, Stellar Systems, and the Sun影响因子(影响力)学科排名




书目名称Cool Stars, Stellar Systems, and the Sun网络公开度




书目名称Cool Stars, Stellar Systems, and the Sun网络公开度学科排名




书目名称Cool Stars, Stellar Systems, and the Sun被引频次




书目名称Cool Stars, Stellar Systems, and the Sun被引频次学科排名




书目名称Cool Stars, Stellar Systems, and the Sun年度引用




书目名称Cool Stars, Stellar Systems, and the Sun年度引用学科排名




书目名称Cool Stars, Stellar Systems, and the Sun读者反馈




书目名称Cool Stars, Stellar Systems, and the Sun读者反馈学科排名

backdrop

人类

978-3-540-12907-3Springer-Verlag Berlin Heidelberg 1984

Crumple

Khaled Khelif,Rose Dieng-Kuntz,Pascal Barbry chromosphere coronae, and extended envelopes which are often characterized by mass loss. Although some manifestations of T Tauri activity can be linked to vigorous solar-stellar phenomena characteristic of cool stars of low mass, other characteristics of T Tauri behavior are exhibited by a wide ran

小步舞

Mike Dean,Yuanbo Guo,Quan Z. Shengncluding the Orion, Taurus-Auriga, ρ Ophiuchi and Chamaeleon clouds obtained with the Einstein X-ray Observatory have revealed more than 150 X-ray luminous PMS stars to date. Some are classical strong emission line T Tauri stars while others are late-type PMS stars with weak or absent lines. The sof

性行为放纵者

性行为放纵者

倾听

W. M. P. van der Aalst,M. Pesicquence is given. From stars of main-sequence spectral type A through early K, the dependence of rotation on mass and age is investigated, from results for stars in open clusters and in the field. The high-mass, single, normal dwarf stars of spectral type A display a common mean projected rotational

beta-cells

Cool Stars, Stellar Systems, and the Sun978-3-540-38785-5Series ISSN 0075-8450 Series E-ISSN 1616-6361

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