Chapter 22 Images

22.1 Milky Way – visible

22.2 Milky Way – infrared

22.3 Milky Way - 21 cm radio

22.4 Milky Way – radio

22.5 Milky Way - X-ray

22.7 Recombination

22.8 HII region development

22.9 The Rosette Nebula, a Classical Hill region

22.10 Hydrogen 21-cm line

22.11 Intercloud gas models

22.18 The Trifid Nebula

22.20 Infrared cirrus

22.21 Interstellar dust

22.22 Herschel's model

22.23 Herschel's explanation

22.24 Two Globular Clusters

22.25 Clusters in Saggitarius

22.26 Cluster distribution

22.27 Galactic coordinates

22.28 Shape of the Milky Way

22.29 Planetary-like rotation

22.30 Milky Way rotation

22.32 The Andromeda galaxy

22.33 Spiral arms near Sun

22.34 Spiral structure

22.35 Spiral structure

22.36 The winding dilemma

22.37 A density wave

22.38 Orbital speed

22.39 Gas cloud motion

22.40 Rotating ring map

22.41 Gas streamers

22.42 Sgr A*

22.43 Gas cloud collisions

22.44 Spiral galaxy NGC 5033

Bonus Image: Milky Way Great Rift

Fix Home Page | Fix 2/e Home Page | Ask the Author Discussion Group | Web Resources

Begin a searchCatalogSiteCampus Rep
MHHE homeabout MHHEhelp desklegal policies and infoorder infowhat's newget involved


Copyright ©1998 The McGraw-Hill Companies. All rights reserved. Any use is subject to the Terms of Use and Privacy Policy. For further information about this site contact mhhe_webmaster@mcgraw-hill.com. McGraw-Hill Higher Education is one of the many fine businesses of The McGraw-Hill Companies.

Corporate Link