The far-infrared signature of dust in high-latitude regions
- 19 November 2003
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 346 (2) , 403-414
- https://doi.org/10.1046/j.1365-2966.2003.07081.x
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- Dust properties of the dark cloud IC?5146Astronomy & Astrophysics, 2003
- Mapping the interstellar dust with near-infrared observations: An optimized multi-band techniqueAstronomy & Astrophysics, 2001
- Far-infrared dust opacity and visible extinction in the Polaris FlareAstronomy & Astrophysics, 2001
- TheCOBEDiffuse Infrared Background Experiment Search for the Cosmic Infrared Background. II. Model of the Interplanetary Dust CloudThe Astrophysical Journal, 1998
- Can Composite Fluffy Dust Particles Solve the Interstellar Carbon Crisis?The Astrophysical Journal, 1997
- IRAS detection of very cold dust in the LYNDS 134 cloud complexThe Astrophysical Journal, 1991
- Variations in the abundance of transiently heated particles within nearby molecular cloudsThe Astrophysical Journal, 1990
- The relationship between infrared, optical, and ultraviolet extinctionThe Astrophysical Journal, 1989
- Star counts and visual extinctions in dark nebulaeThe Astronomical Journal, 1978
- Palomar Schmidt star counts for 2 heavily obscured fields.The Astronomical Journal, 1956