Spiral arms, bar shape and bulge microlensing in the Milky Way
Open Access
- 1 March 2002
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 330 (3) , 591-608
- https://doi.org/10.1046/j.1365-8711.2002.05116.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 28 references indexed in Scilit:
- Three‐dimensional Structure of the Milky Way Disk: The Distribution of Stars and Dust beyond 0.35R⊙The Astrophysical Journal, 2001
- The MACHO Project: Microlensing Results from 5.7 Years of Large Magellanic Cloud ObservationsThe Astrophysical Journal, 2000
- The MACHO Project: Microlensing Optical Depth toward the Galactic Bulge from Difference Image AnalysisThe Astrophysical Journal, 2000
- Is Galactic Structure Compatible with Microlensing Data?The Astrophysical Journal, 2000
- Proper Motion of the Compact, Nonthermal Radio Source in the Galactic Center, Sagittarius A*The Astrophysical Journal, 1999
- Gas dynamics and large-scale morphology of the Milky Way galaxyMonthly Notices of the Royal Astronomical Society, 1999
- The microlensing optical depth of the COBEbulgeMonthly Notices of the Royal Astronomical Society, 1997
- The photometric structure of the inner GalaxyMonthly Notices of the Royal Astronomical Society, 1997
- On the deprojection of the Galactic bulgeMonthly Notices of the Royal Astronomical Society, 1996
- Direct evidence for a bar at the Galactic centerThe Astrophysical Journal, 1991