Image Details
Caption: Fig. 3.
(a)–(e) Spectra of FU Ori stars taken with the UKIRT CGS3 low‐resolution grating. Model fits are described in the text and are summarized in Tables 2 and 3. V1057 Cyg was observed in 1992 and 1993; the model fits were done for the 1993 spectrum.
© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.