Slide 1 ASTR112 The Galaxy Lecture 3 Prof. John Hearnshaw 5. Stellar populations 6. Galactic (open) clusters The Pleiades open cluster Slide 2 ASTR112 The Galaxy Lecture…
Slide 1Please press “1” to test your transmitter. :10 0 of 5 1.1 2.2 3.3 4.4 5.5 Review for Midterm II 1234567891011121314151617181920 2122232425262728293031323334353637383940…
Slide 1 Slide 2 Still contains your circumpolar constellations: Ursa Major, Ursa Minor, Cepheus, Cassiopeia and Draco Summer constellations, such as Cygnus, Aquila and Lyra,…
Slide 1 Radio Astronomy And The Spiral Structure Of The Milky Way Jess Broderick Supervisor: Dr George Warr Slide 2 Outline Overview of the spiral arm structure of the…
Slide 1 Chapter 16: Star Formation What force makes stars? Gravity! Out of what? Interstellar gas and dust But this stuff is VERY low density… a dense area may have ~100…
Radio Astronomy And The Spiral Structure Of The Milky Way Jess Broderick Supervisor: Dr George Warr Outline Overview of the spiral arm structure of the Milky Way. Using radio…
Stellar Evolution â the Life and Death of a Star⦠Hereâs the Story Weâll Unfold for you⦠Formation in giant molecular clouds Fusion halts collapse, stabilizes star…
Inter Stellar Matter with a high enough density, and a low enough temperature for proto-stars to form. Protostars form in cold dark nebulae Star Formation Giant Molecular…
Inter Stellar Matter with a high enough density, and a low enough temperature for proto-stars to form. Protostars form in cold dark nebulae Star Formation Giant Molecular…
MLO as Viewed from Wooded Hill Cleveland National Forest 45 air miles east of San Diego 40â 21â 50â (in progress) 24â HPWREN Antenna Upgrade of âIllinoisâ 40-inch NSF:…