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Are gaint planets forming around HR 4796A?We have obtained Far Ultraviolet Spectroscopic Explorer and Hubble Space Telescope STIS spectra of HR 4796A, a nearby 8 Myr old main-sequence star that possesses a dusty circumstellar disk whose inclination has been constrained from high-resolution near-infrared observations to be 17 degrees from edge-on.
Document ID
20060029372
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/7988
Authors
Chen, C. H.
Kamp, I.
Date Acquired
August 23, 2013
Publication Date
February 1, 2004
Publication Information
Publication: Astrophysical Journal
Volume: 602
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
circumstellar matter planetary systems stars

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