Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999apj...514l.115s&link_type=abstract
The Astrophysical Journal, Volume 514, Issue 2, pp. L115-L119.
Astronomy and Astrophysics
Astronomy
55
Stars: Circumstellar Matter, Ism: Planetary Nebulae: General, Stars: Agb And Post-Agb, Stars: Mass Loss
Scientific paper
We present Hubble Space Telescope (HST) Wide-Field and Planetary Camera 2 images and VLA OH maser emission-line maps of the cold infrared object IRAS 16342-3814, believed to be a protoplanetary nebula. The HST images show an asymmetrical bipolar nebula, with the lobes separated by a dark equatorial waist. The two bright lobes and the dark waist are simply interpreted as bubble-like reflection nebulae illuminated by starlight escaping through polar holes in a dense, flattened, optically thick cocoon of dust, which completely obscures the central star. A faint halo can be seen surrounding each of the lobes. The bubbles are likely to have been created by a fast outflow (evidenced by H_2O emission) plowing into a surrounding dense, more slowly expanding, circumstellar envelope of the progenitor asymptotic giant-branch (AGB) star (evidenced by the halo). The IRAS fluxes indicate a circumstellar mass of about 0.7 M_solar(D/2 kpc) and an AGB mass-loss rate of about 10^-4 M_solar yr^-1 (V_exp/15 km s^-1)(D/2 kpc)^2 (assuming a gas-to-dust ratio of 200). OH features with the largest redshifted and blueshifted velocities are concentrated around the bright eastern and western polar lobes, respectively, whereas intermediate-velocity features generally occur at low latitudes, in the dark waist region. We critically examine evidence for the post-AGB classification of IRAS 16342-3814.
Likkel Lauren
Morris Mark
Sahai Raghvendra
te Lintel Hekkert Peter
Zijlstra Albert
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