High-resolution mapping of mass loss from highly evolved carbon stars

Details High-resolution mapping of mass loss from highly evolved carbon stars High-resolution mapping of mass loss from highly evolved carbon stars

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986inpr.conf...63b&link_type=abstract

In NASA. Ames Research Center Summer School on Interstellar Processes: Abstracts of Contributed Papers p 63-64 (SEE N87-15043 0

Computer Science

Carbon Stars, Losses, Mapping, Planetary Nebulae, Stellar Mass, Cosmic Dust, Interferometry, Photodissociation, Radiation Pressure, Stellar Winds

Scientific paper

The molecular component of the mass outflow at high resolution was mapped with the Owens Valley Millimeter-Wave Interferometer in two well-known objects, CRL 2688 and CIT 6. Interferometric observations of a pair of carbon stars which are evolving toward the planetary nebula stage have revealed evidence of episodic, nonspherically symmetric mass loss, and may lead to a fuller understanding of shielding properties of the dust grains involved in these flows.

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