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

CHORD

書目名稱Cool Stars, Stellar Systems, and the Sun影響因子(影響力)




書目名稱Cool Stars, Stellar Systems, and the Sun影響因子(影響力)學科排名




書目名稱Cool Stars, Stellar Systems, and the Sun網(wǎng)絡公開度




書目名稱Cool Stars, Stellar Systems, and the Sun網(wǎng)絡公開度學科排名




書目名稱Cool Stars, Stellar Systems, and the Sun被引頻次




書目名稱Cool Stars, Stellar Systems, and the Sun被引頻次學科排名




書目名稱Cool Stars, Stellar Systems, and the Sun年度引用




書目名稱Cool Stars, Stellar Systems, and the Sun年度引用學科排名




書目名稱Cool Stars, Stellar Systems, and the Sun讀者反饋




書目名稱Cool Stars, Stellar Systems, and the Sun讀者反饋學科排名

backdrop

人類

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

性行為放縱者

性行為放縱者

傾聽

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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