Radiative transfer in disc galaxies -- III. The observed kinematics of dusty disc galaxies
Open Access
- 21 August 2003
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 343 (4) , 1081-1094
- https://doi.org/10.1046/j.1365-8711.2003.06770.x
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This publication has 48 references indexed in Scilit:
- The Hernquist model revisited: Completely analytical anisotropic dynamical modelsAstronomy & Astrophysics, 2002
- Kinematics of elliptical galaxies with a diffuse dust component – III. A Monte Carlo approach to include the effects of scatteringMonthly Notices of the Royal Astronomical Society, 2002
- Dark Matter Halos around Elliptical Galaxies: How Reliable Is the Stellar Kinematical Evidence?The Astrophysical Journal, 2001
- Radiative transfer in disc galaxies - I. A comparison of four methods to solve the transfer equation in plane-parallel geometryMonthly Notices of the Royal Astronomical Society, 2001
- The dark matter distribution in disc galaxiesMonthly Notices of the Royal Astronomical Society, 2001
- Accurate Determination of the Mass Distribution in Spiral Galaxies. II. Testing the Shape of Dark HalosThe Astronomical Journal, 2001
- Kinematics of elliptical galaxies with a diffuse dust component - II. Dust effects on kinematic modellingMonthly Notices of the Royal Astronomical Society, 2000
- Kinematics of elliptical galaxies with a diffuse dust componentMonthly Notices of the Royal Astronomical Society, 2000
- Effects of clumping on the observed properties of dusty galaxiesMonthly Notices of the Royal Astronomical Society, 2000
- Monte Carlo Simulations of Dusty Spiral Galaxies: Extinction and Polarization PropertiesThe Astrophysical Journal, 1996