Accretion Processes in T Tauri Stars: GHRS Observations

Details Accretion Processes in T Tauri Stars: GHRS Observations Accretion Processes in T Tauri Stars: GHRS Observations

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003csss...12..723a&link_type=abstract

The Future of Cool-Star Astrophysics: 12th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (2001 July 30 - August

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have performed observations of eight classical and one weak T Tauri
Star, using the GHRS instrument on board of HST. We observe the
ion{Si}{4} (1400 Å), ion{C}{4} (1550 Å), and ion{Mg}{2}
(2800 Å) resonance doublets, and numerous H2 lines.
Here we discuss the observational characteristics of these lines.

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