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Ïîèñêîâûå ñëîâà: diurnal motion

Determinations of Dust Scattering Properties from Dark Clouds

Interstellar Dust Scattering Properties from Dark Clouds

From K. D. Gordon 2004, in "Astrophysics of Dust", (ASP Conf. Proceed. 196), ed. A. N. Witt, G. C. Clayton, & B. T. Draine, (ASP: San Francisco), 77

Updated: KDG - 28 Nov 2006

Single Scattering Albedo a	Scattering Phase Function Asymmetry g = < cos(α) >
Dark Cloud Plots

ASCII file of plotted data

Reference	Description	Model Type	In Plot	Comment
Dark Cloud Studies
Matilla 1970	Coalsack and dark cloud in Libra; UBV	DC1	Yes
Fitzgerald et al. 1976	Thumbprint Nebula; B	DC1	Yes
Laureijs et al. 1987	L1642; 3500 - 5500 Å	DC1	Yes	No g determination possible
Witt et al. 1990	Bok globule; 4690, 6500, & 8560 Å	DC1	Yes
Hurwitz 1994	Taurus molecular cloud; Berkeley UVX 1600 Å	DC2	Yes
Haikala et al. 1995	G251.2+73.3 cirrus cloud; FAUST 1400-1800 Å	DC1	Yes
Lehtinen & Mattila 1996	Thumbprint Nebula; JHK	DC1	Yes	No g determination possible

Name	Description
Radiative Transfer Models
DC1	Monte Carlo; MW ISRF & specific stars; homogeneous sphere
DC2	Numerical int.; MW ISRF; 2D distribution

References

Interstellar dust scattering properties from: [Diffuse Galactic Light] [Reflection Nebulae] [Dark Clouds]