Physics
Scientific paper
Jul 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat..41140341g&link_type=abstract
VizieR On-line Data Catalog: J/A+AS/114/341. Originally published in: 1995A&AS..114..341G
Physics
Photometry: Ubv, Photometry: Ubvri
Scientific paper
In this paper we present the results of a long campaign of coordinated (sometimes simultaneous) multifrequency observations, from X-ray to radio wavelengths of the extreme T Tauri star RU Lupi. The large amount of data obtained can be useful to understanding the physics governing the intriguing behaviour of this pre-main-sequence star. In particular, from the whole set of data, a model with a protoplanetary accretion disk around a moderately magnetic star seems to be the most promising picture for this source. (3 data files).
Bisnovatyi-Kogan Gennadi S.
Errico L.
Giovannelli Franco
Kurt Victoria G.
Lamzin Sergei A.
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