Is it possible to observe the emission from the boundary layers of FU Ori stars?

Details Is it possible to observe the emission from the boundary layers of FU Ori stars? Is it possible to observe the emission from the boundary layers of FU Ori stars?

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997astl...23..604e&link_type=abstract

Astronomy Letters, Volume 23, Issue 5, September 1997, pp.604-608; Pis'ma v Astronomicheskii Zhurnal, Vol. 23, p. 687

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Our estimates show that the optical depth of the stellar wind from the
FU Ori stars FU Ori, V1057 Cyg, and Z CMa in the Balmer and Paschen
contunua can be greater than unity. It is probably for this reason that
no optical and ultraviolet emission is observed from the innermost and
hottest regions of these objects the boundary layers of accretion disks.

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