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WFPC2 Imaging of the Circumstellar Nebulosity of HL TauriHL Tauri is considered a prototype solar-mass T Tauri star. Planetary camera images of HL Tauri have been obtained through V, R, and I band filters using the Wide Field Planetary Camera 2 aboard the refurbished Hubble Space Telescope. These images show that HL Tauri is entirely reflection nebulosity at optical wavelengths, with no optical star visible to a limiting magnitude of V=25.5.
Document ID
20060037213
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Stapelfeldt, K. R.
Burrows, C. J.
Krist, J. E.
Trauger, J. T.
Hester, J. J.
Holtzman, J. A.
Ballester, G. E.
Casertano, S.
Clarke, J. T.
Crisp, D.
Evans, R. W.
III, J. S. Gallagher
Griffiths, R. E.
Hoessel, J. G.
Mould, J. R.
Scowen, P. A.
Watson, A. M.
Westphal, J. A.
Date Acquired
August 23, 2013
Publication Date
January 1, 1995
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
circumstellar matter stars HL Tauri pre-main sequence astrophysics

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