An icy, bipolar pre-planetary nebula with knotty jets: IRAS 22036+5306
Sahai R., Zijlstra A.A., Sanchez-Contreras C., Morris M., 2003, ApJL,
586, L81
Abstract
Using the Hubble Space Telescope's Wide Field Planetary Camera 2, we
have discovered that the proto-planetary nebula (PPN) IRAS 22036+5306
(I22036) is an extended (5.7"×1.3") bipolar nebula. A dark,
(partial) ringlike band defines the nebular waist region and probably
results from a tilted, geometrically thick disk that obscures the
central star. Knotty, linear structures are seen in each lobe. Very
Large Array A configuration observations of OH maser emission in I22036
show the 1667 MHz emission features aligned in a roughly 1.8 arcsec long
linear structure along the nebular axis. The source's far-infrared
fluxes imply the presence of a massive [~5(D/2 kpc)2
Msolar], dusty, cool (Tdust~35-67 K),
circumstellar envelope. Strong 3.08 and 11 μm absorption features in
the Infrared Space Observatory spectra show the presence of icy silicate
grains, which probably reside in the disk's shielded outer regions. A
low-resolution optical spectrum indicates an F5 (or earlier) spectral
type for the post-asymptotic giant branch (AGB) central star and shows
Hα and Hβ emission lines. The elongated and highly structured
lobes of I22036 are likely to have been produced as a result of the
interaction of a collimated, fast wind (CFW) with the AGB progenitor's
dense, slow wind. Highly collimated jetlike components in the CFW have
probably operated at some time during the formation of this PPN.
paper (pdf, 330kb)