✦ LIBER ✦

Rotational evolution of solar-type stars

✍ Scribed by V. S. Geroyannis; G. A. Antonakopoulos

Publisher: Springer Netherlands
Year: 1981
Tongue: English
Weight: 628 KB
Volume: 79
Category: Article
ISSN: 0004-640X
DOI: 10.1007/bf00649433

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Determination of the rotational excitati

Determination of the rotational excitation temperature in solar type stars

✍ M. J. Fernández-Figueroa; M. Rego; A. Perea 📂 Article 📅 1982 🏛 Springer Netherlands 🌐 English ⚖ 300 KB

Rotation and activity in the solar-type

Rotation and activity in the solar-type stars of NGC 2547

✍ R. D. Jeffries; E. J. Totten; D. J. James 📂 Article 📅 2000 🏛 John Wiley and Sons 🌐 English ⚖ 403 KB

Mass loss from solar-type stars

✍ L. Hartmann 📂 Article 📅 1985 🏛 Springer 🌐 English ⚖ 656 KB

Winds are directly detected from solar-type stars only when they are very young. At ages ~ 106 yr, these stars have mass loss rates ~ 106 times the mass flux of the present solar wind. Although these young T Tauri stars exhibit ultraviolet transition-region and X-ray coronal emission, the large part

Stellar evolution and late type stars

✍ T. Lloyd Evans 📂 Article 📅 1995 🏛 Springer Netherlands 🌐 English ⚖ 583 KB

Rotational mixing in early-type main-seq

Rotational mixing in early-type main-sequence stars

✍ Ian D. Howarth; Keith C. Smith 📂 Article 📅 2001 🏛 John Wiley and Sons 🌐 English ⚖ 692 KB

Comparison of UV spectra from solar-type

Comparison of UV spectra from solar-type stars

✍ A. Greve; W. Wamsteker 📂 Article 📅 1984 🏛 Springer 🌐 English ⚖ 415 KB

We compare high-resolution spectra from the Sun and the four solar-type stars 16 CygA, 16 Cyg B, HD 32008, HD 34411 obtained with IUE in the wavelength range 2650-2930 A. The comparison is made for peak intensities between absorption lines. At the level of accuracy of the IUE observations, the stars