Vla And Sma Observations Of The Young Planetary Nebula Iras 17347-3139

Details Vla And Sma Observations Of The Young Planetary Nebula Iras 17347-3139 Vla And Sma Observations Of The Young Planetary Nebula Iras 17347-3139

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21335903t&link_type=abstract

American Astronomical Society, AAS Meeting #213, #359.03; Bulletin of the American Astronomical Society, Vol. 41, p.502

Astronomy and Astrophysics

Astronomy

Scientific paper

IRAS 17347-3139 is one of the three planetary nebulae that are known to harbor water maser emission, suggesting that it has just entered the planetary nebula phase. In this work we present radio interferometric observations of the radio continuum at centimetric wavelengths (carry out with the Very Large Array of the NRAO), and the CO emission at millimetric wavelengths (carry out with the Sub Millimeter Array of the SAO & ASIAA).
From our observations we have resolved for the first time the ionized as well as the molecular component of this planetary nebula. We propose that a collimated precessing wind could be excavating the neutral component producing the bipolar morphology observed in this interesting object.

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