Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.stsci.edu/~kgordon/Dust/Scat_Param/scat_data_rn.html
Äàòà èçìåíåíèÿ: Tue Nov 28 20:01:01 2006
Äàòà èíäåêñèðîâàíèÿ: Tue May 27 07:51:34 2008
Êîäèðîâêà:
Ïîèñêîâûå ñëîâà: asteroid

Determinations of Dust Scattering Properties from Reflection Nebulae

Interstellar Dust Scattering Properties from Reflection Nebulae

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) >
Reflection Nebulae Plots

ASCII file of plotted data

Reference	Description	Model Type	In Plot	Comment
Reflection Nebulae Studies
Witt et al. 1982	NGC 7023; IUE 1200 - 3000 Å & ground-based 3470 - 5515 Å	RN1	Partial	UV determinations of g not included (not enough data for both a & g in UV)
Witt et al. 1992	NGC 7023; UIT 1400 - 2800 Å	RN1	Yes
Witt et al. 1993	NGC 7023; Voyager 2 1000 - 1300 Å	RN1	Yes
Gordon et al. 1994	Sco OB2; 1362 & 1769 Å	RN2	Yes
Calzetti et al. 1995	IC 435; IUE 1200 - 3100 Å & ground-based BV	RN1	Yes
Burgh et al. 2002	NGC 2023; FOT 900 - 1400 Å	RN1	Yes
Gibson & Nordsieck 2003	Pleiades; WISP 1650 & 2200 Å;	RN3	Yes
Shalima & Murphy 2006	Orion; FUSE	RN4	Yes

Name	Description
Radiative Transfer Models
RN1	Monte Carlo; single star; homogeneous sphere
RN2	Monte Carlo; multiple stars; homogeneous sphere
RN3	analytic single scattering; multiple stars; approximated clumpy slab
RN4	Monte Carlo; foreground slab

References

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