Optical, infrared and millimetre-wave properties of Vega-like systems.

Details Optical, infrared and millimetre-wave properties of Vega-like systems. Optical, infrared and millimetre-wave properties of Vega-like systems.

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.279..915s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. Vol. 279, No. 3, p. 915 - 939

Astronomy and Astrophysics

Astronomy

150

Circumstellar Matter -- Stars: Evolution -- Planetary Systems -- Infrared: Stars, Circumstellar Shells: Ubvri Photometry, Circumstellar Shells: Infrared Photometry, Circumstellar Shells: Infrared Spectra, Circumstellar Shells: Sub-Mm Radiation, Circumstellar Shells: Mm Radiation

Scientific paper

Vega-like stars are main-sequence stars that exhibit excess infrared emission due to dust grains which are believed to be distributed in circumstellar discs. To facilitate modelling of the properties of the discs and of their constituent grains, the authors have assembled and discuss a new observational database for a large sample of candidate Vega-like systems, which comprises UBVRI optical photometry, JHKLL'M near-IR photometry, mid-IR spectra, and mm/submm-wave photometry.

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