✦ LIBER ✦

Detection of optical circular polarization in the Herbig Ae star WW Vul

✍ Scribed by D. N. Shakhovskoi; O. S. Shulov; E. N. Kopatskaya

Book ID: 110126971
Publisher: Springer
Year: 2001
Tongue: English
Weight: 45 KB
Volume: 27
Category: Article
ISSN: 1063-7737
DOI: 10.1134/1.1374675

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Dust around young stars. Model of envelo

Dust around young stars. Model of envelope of the Ae Herbig star WW Vul

✍ N. V. Voshchinnikov; V. P. Grinin 📂 Article 📅 1992 🏛 Springer 🌐 English ⚖ 967 KB

Anomalous Behavior of the Linear Polariz

Anomalous Behavior of the Linear Polarization of the Herbig Ae Star WW Vul during the 1997 Minimum

✍ D. N. Shakhovskoi 📂 Article 📅 2002 🏛 Springer 🌐 English ⚖ 89 KB

Structure of the inner regions of the ci

Structure of the inner regions of the circumstellar gas envelopes of young hot stars. I. The isolated Ae Herbig star WW Vul

✍ O. V. Kozlova; D. N. Shakhovskoi; A. N. Rostopchina; I. Yu. Alekseev 📂 Article 📅 2006 🏛 Springer 🌐 English ⚖ 228 KB

Rapid variability of the line He I λ 587

Rapid variability of the line He I λ 587.6 nm in the spectrum of the Herbig Ae/Be star WW Vul

✍ A. F. Pugach 📂 Article 📅 2007 🏛 Allerton Press Inc 🌐 English ⚖ 87 KB

Search for periodicity in light variatio

Search for periodicity in light variations of the isolated Herbig Ae-star WW Vulpeculae

✍ N. A. Volchkova 📂 Article 📅 1993 🏛 Springer 🌐 English ⚖ 250 KB

The exceptional Herbig Ae star HD 101412

The exceptional Herbig Ae star HD 101412: The first detection of resolved magnetically split lines and the presence of chemical spots in a Herbig star

✍ S. Hubrig; M. Schöller; I. Savanov; J.F. Gonzälez; C.R. Cowley; O. Schütz; R. Ar 📂 Article 📅 2010 🏛 John Wiley and Sons 🌐 English ⚖ 380 KB

## Abstract In our previous search for magnetic fields in Herbig Ae stars, we pointed out that HD 101412 possesses the strongest magnetic field among the Herbig Ae stars and hence is of special interest for follow‐up studies of magnetism among young pre‐main‐sequence stars. We obtained high‐resolut