'Clumps' presentation slideshows

Structure Formation in Tidal Tails

660 views • 44 slides

Mining Hot, Luminous Stars in the Southern Sky: A New Look at the Magellanic-Cloud System

375 views • 25 slides

Life Cycle of a Star

330 views • 23 slides

Structure, star formation and magnetic fields in the OMC 1 region

Structure, star formation and magnetic fields in the OMC 1 region. Coppin et al., A&A, 356, 1031 (2000). UMEKAWA Michihisa (ASAFAS). Plasma seminar Feb. 2. Observation of OMC1 using 450 and 850 micro m clump mass function polarimetry (direction of magnetic fields).

348 views • 22 slides

Chapter 29 Exploring the Early Universe

Chapter 29 Exploring the Early Universe. Guiding Questions. Has the universe always expanded as it does today? What is antimatter? How can it be created, and how is it destroyed? Why is antimatter so rare today?

428 views • 18 slides

The life cycle of a star

Science 9 . The life cycle of a star. Gravity is a force that pulls objects toward each other The more mass an object has, the more gravity it exerts The Sun has stronger gravity than Earth The force gets smaller as the distance between two objects increases

305 views • 18 slides

Soil

259 views • 11 slides