DLAP questions | universe10e_ch22_1_dlap.xml | 534c6bf8757a2e4a30000002 |
22-1 The Sun is located in the disk of our Galaxy, about 8000 parsecs from the galactic center
| universe10e_ch22_2.html | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_2_dlap.xml | 534c6bf8757a2e4a30000002 |
22-2 Observations at nonvisible wavelengths reveal the shape of the Galaxy
| universe10e_ch22_3.html | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_3_dlap.xml | 534c6bf8757a2e4a30000002 |
22-3 Observations of cold hydrogen clouds and star-forming regions reveal that our Galaxy has spiral arms
| universe10e_ch22_4.html | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_4_dlap.xml | 534c6bf8757a2e4a30000002 |
22-4 The rotation of our Galaxy reveals the presence of dark matter
| universe10e_ch22_5.html | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_5_dlap.xml | 534c6bf8757a2e4a30000002 |
22-5 Spiral arms are caused by density waves that sweep around the Galaxy
| universe10e_ch22_6.html | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_6_dlap.xml | 534c6bf8757a2e4a30000002 |
22-6 Infrared, radio, X-ray, and gamma-ray observations are used to probe the galactic center
| universe10e_ch22_7.html | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_7_dlap.xml | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_8_dlap.xml | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_9_dlap.xml | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_10_dlap.xml | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_11_dlap.xml | 534c6bf8757a2e4a30000002 |
DLAP questions | universe10e_ch22_12_dlap.xml | 534c6bf8757a2e4a30000002 |