University of Hertfordshire

From the same journal

By the same authors

  • M. Takami
  • A. Chrysostomou
  • J. Bailey
  • T. Gledhill
  • M. Tamura
  • H. Terada
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Original languageEnglish
Pages (from-to)143-146
JournalAstrophysics and Space Science
Volume287
Issue1-4
DOIs
Publication statusPublished - 2003

Abstract

Jets and winds in pre-main sequence (PMS) stars are often heated and ionized, and understanding their heating mechanism is desired to compare UV-to-IR spectral signatures with models and thus investigate their driving mechanism. We review our results of long-slit spectroscopy and spectro-astrometry for He I 1.083 μm and Hα emission, and investigate the heating mechanisms in the jet in the outer (>10 AU) and inner (<10 AU) regions, respectively.

Notes

The original publication is available at www.springerlink.com Copyright Springer [Full text of this article is not available in the UHRA]

ID: 181888