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Dive into the components and structure of our own galaxy, the Milky Way, from its central Sun to globular clusters, extinction, molecular clouds, and more. Learn about its kinematics, rotation curve, and gravitational microlensing method.
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PX269 Galaxies Part 2: Our Galaxy, the Milky Way 2.1 Components and Structure PX269 Galaxies
The Milky Way Wei-Hao Wang University of Hawaii
First map of Milky Way: Sun near centre Herschel, 1785
The Milky Way Wei-Hao Wang University of Hawaii
Kapteyn, 1922 Star counts with distance scale
Shapley & Shapley, 1919 Distribution of globular clusters
Wei-Hao Wang University of Hawaii Extinction in plane of Milky Way
NGC 6744, Milky Way-like galaxy Capella Observatory
Wei-Hao Wang University of Hawaii Extinction in plane of Milky Way
Pleiades open cluster Scattered light Philip Perkins
NGC 891 Optical Infra-red 2MASS CFHT
Wei-Hao Wang University of Hawaii
M 51 the Whirlpool Galaxy HII regions
Optical spectrum of an HII region Diaz et al 1987 Flux Wavelength (Angstroms)
HII regions: the Orion Nebula Mike Fleenor
NGC 6744, Milky Way-like galaxy Capella Observatory
Part 2: Our Galaxy, the Milky Way 2.2 Kinematics
Galactic co-ordinates Carroll & Ostlie, 1996
21 cm line profile along one line of sight Carroll & Ostlie, 1996
A = rotation curve for centrally-concentrated mass distribution B = rotation curve for extended mass distribution
The Milky Way Wei-Hao Wang University of Hawaii
First detection of a gravitational microlensing event Alcock et al 1993