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| Query : 2004MNRAS.352.1319S |
2004MNRAS.352.1319S - Mon. Not. R. Astron. Soc., 352, 1319-1322 (2004/August-3)
Modelling of dust scattering toward the Coalsack.
SHALIMA P. and MURTHY J.
Abstract (from CDS):
Murthy, Henry & Holberg discovered intense far-ultraviolet (FUV) (λλ912-1600) emission from the direction of the Coalsack molecular cloud 10 years ago. We have used their results in conjunction with a Monte Carlo model for the scattering in the region to show that the scattering is from dust in the foreground of the Coalsack. The albedo of the grains is 0.4±0.2. This is one of the few determinations of the albedo of dust in the diffuse interstellar medium in the FUV.
Abstract Copyright: 2004 RAS
Journal keyword(s): dust, extinction - ultraviolet: ISM
Simbad objects: 4
| Number of rows : 4 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | * alf Cru | SB* | 12 26 35.89522 | -63 05 56.7343 | B0.5IV+B1V | 99 | 0 | |||||
| 2 | NAME Coalsack Nebula | DNe | 12 31 19 | -63 44.6 | ~ | 275 | 0 | |||||
| 3 | * bet Cru | bC* | 12 47 43.26877 | -59 41 19.5792 | 0.03 | 1.02 | 1.25 | 1.38 | 1.64 | B1IV | 360 | 1 |
| 4 | * bet Cen | bC* | 14 03 49.40535 | -60 22 22.9266 | 0.58 | B1III | 371 | 0 |
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