A 500kms-1 outflow from the young bipolar planetary nebula Mz 3

Details A 500kms-1 outflow from the young bipolar planetary nebula Mz 3 A 500kms-1 outflow from the young bipolar planetary nebula Mz 3

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mnras.312l..23r&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 312, Issue 2, pp. L23-L27.

Astronomy and Astrophysics

Astronomy

25

Circumstellar Matter, Ism: Jets And Outflows, Planetary Nebulae: General, Planetary Nebulae: Individual: Mz 3 (Pn G331.7-01.0), Ism: Structure

Scientific paper

We report the discovery of a pair of hypersonic (~=+/-500kms-1) velocity features located along the bipolar axis of the young planetary nebula Mz 3. The possible physical mechanisms that can produce such extreme outflows are briefly discussed and compared with mechanisms thought to operate in MyCn 18, He 2-111 and KjPn 8, all of which exhibit equally remarkable hypersonic outflows of differing kinds.

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