Millimetre continuum observations of low-mass carbon-rich stars

Details Millimetre continuum observations of low-mass carbon-rich stars Millimetre continuum observations of low-mass carbon-rich stars

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.273..906s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 273, Issue 4, pp. 906-912.

Astronomy and Astrophysics

Astronomy

11

Stars: Carbon, Circumstellar Matter, Stars: Individual: 89 Her, Stars: Individual: Ac Her, Infrared: Stars, Radio Continuum: Stars

Scientific paper

We present millimetre continuum observations of the low-mass,
carbon-rich stars 89 Her and AC Her. The IRAS-millimetre flux
distributions are consistent with emission by large (>~1 μm)
grains. This suggests that the grains are confined in the circumstellar
environment rather than participating in an outflow.

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