Gas dynamics in the Milky Way: second pattern speed and large-scale morphology
Open Access
- 11 April 2003
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 340 (3) , 949-968
- https://doi.org/10.1046/j.1365-8711.2003.06358.x
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This publication has 35 references indexed in Scilit:
- Spiral arms, bar shape and bulge microlensing in the Milky WayMonthly Notices of the Royal Astronomical Society, 2002
- Proper Motion of the Compact, Nonthermal Radio Source in the Galactic Center, Sagittarius A*The Astrophysical Journal, 1999
- The photometric structure of the inner GalaxyMonthly Notices of the Royal Astronomical Society, 1997
- A self-consistent model of the spiral structure of the GalaxyMonthly Notices of the Royal Astronomical Society, 1997
- The existence and shapes of dust lanes in galactic barsMonthly Notices of the Royal Astronomical Society, 1992
- Understanding the kinematics of Galactic Centre gasMonthly Notices of the Royal Astronomical Society, 1991
- The rotation of the Galaxy within the solar circleThe Astrophysical Journal, 1990
- Massachusetts-Stony Brook Galactic plane CO survey - The Galactic disk rotation curveThe Astrophysical Journal, 1985
- Does the Galaxy have four spiral armsThe Astrophysical Journal, 1981
- On the dynamics of agglomerating ensembles of cloudsThe Astrophysical Journal, 1980