Optical, infrared and millimetre-wave properties of Vega-like systems - III. Models with thermally spiking grains

Monthly Notices of the Royal Astronomical Society

Volumn 289, Issue 4, 1997, Pages 831-846

  Sylvester, R J ^a   Skinner, C J ^b   Barlow, M J ^a  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b STScI   (United States)

Author keywords

Circumstellar matter; Infrared: Stars; Planetary systems

Indexed keywords

DUST; LUMINANCE; MILLIMETER WAVES; RADIATIVE TRANSFER; THERMODYNAMICS;

CIRCUMSTELLAR MATTERS; DUST GRAINS; INFRARED: STAR; IR SPECTRUM; IR WAVELENGTHS; LONG WAVELENGTH; NEAR-IR; OPTICAL-; PLANETARY SYSTEM; THERMAL-EQUILIBRIUM;

STARS;

EID: 0012954653     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/289.4.831     Document Type: Article

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