Variable circumstellar obscuration of the carbon star R Fornacis

Details Variable circumstellar obscuration of the carbon star R Fornacis Variable circumstellar obscuration of the carbon star R Fornacis

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..331f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Nov. 15, 1984, p. 331-337.

Astronomy and Astrophysics

Astronomy

29

Carbon Stars, Stellar Envelopes, Stellar Occultation, Variable Stars, Absorption Spectra, Graphite, Infrared Spectra, Light Curve, Mira Variables, Particle Size Distribution, Radiant Flux Density, Stellar Spectrophotometry, Visible Spectrum

Scientific paper

In 1983, the carbon Mira-type variable R For became unusually faint in
the visible and infrared. This is interpreted as a change in
circumstellar obscuration. For absorption by graphite spheres, the
required particle radius is 0.15 microns.

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