Hostname: page-component-54dcc4c588-r5qjk Total loading time: 0 Render date: 2025-10-01T18:41:42.286Z Has data issue: false hasContentIssue false
  • English
  • Français

Imaging the Surface of a Star: VLBA Monitoring of the SiO Masers around U Herculis

Published online by Cambridge University Press:  12 April 2016

P. J. Diamond  and
A. J. Kemball
P. J. Diamond
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, USA
A. J. Kemball
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We report on 4 epochs of VLBA polarization observations of the 43 GHz, v=1, J=1–0 SiO masers in the circumstellar envelope around the Mira variable U Herculis.

Information

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 245 - 246
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Boboltz, D.A., et al. 1997. ApJ, 487 L147–150.CrossRefGoogle Scholar
Diamond, P.J., et al. 1994. ApJ, 430, L61–65.CrossRefGoogle Scholar
Kemball, A.J. & Diamond, P.J. 1997. ApJ, 481, Llll–114.CrossRefGoogle Scholar