Effects of clumping on the observed properties of dusty galaxies
Open Access
- 21 January 2000
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 311 (3) , 601-610
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This publication has 18 references indexed in Scilit:
- Whence the Local Bubble, Gum, Orion? GSH 238+00+09, A Nearby Major Superbubble toward Galactic Longitude 238oThe Astrophysical Journal, 1998
- The Five College Radio Astronomy Observatory CO Survey of the Outer GalaxyThe Astrophysical Journal Supplement Series, 1998
- Dust in Starburst GalaxiesThe Astrophysical Journal, 1997
- Diagnostics of dust content in spiral galaxies: Numerical simulations of radiative transferThe Astrophysical Journal, 1994
- Radiative transfer in a clumpy medium - I. Analytical Markov-process solution for an N-phase slabMonthly Notices of the Royal Astronomical Society, 1993
- Distribution of CO in the Milky WayAnnual Review of Astronomy and Astrophysics, 1991
- The gas/dust ratio in spiral galaxiesThe Astrophysical Journal, 1990
- Are galaxy discs optically thick?Monthly Notices of the Royal Astronomical Society, 1989
- The universe at faint magnitudes. I - Models for the galaxy and the predicted star countsThe Astrophysical Journal Supplement Series, 1980
- Diffuse radiation in the GalaxyThe Astrophysical Journal, 1941