1. arXiv:astro-ph/0107111v15Jul2001 X-rays and Protostars in the Trifid Nebula Jeonghee Rho Infrared Processing and Analysis Center, California Institute of Technology,…

Slide 1Stellar Rotation in the CoRoT Era Jose Dias do Nascimento Jr & José Renan de Medeiros and team DFTE- Natal Departamento de Física Teórica e Experimental, Brazil…

Slide 1Protostellar/planetary disk observations (and what they might imply) Lee Hartmann University of Michigan Slide 2 What do we want to know? What are disk masses? How…

Slide 1Accretion Processes in Star Formation Lee Hartmann Cambridge Astrophysics Series, 32 Cambridge University Press (also from Nuria Calvet talks (2004) (continued) Slide…

Slide 1Image credit: NASA, ESA and A. Evans (Stony Brook University, New York) Probing the evolution of merger remnants via formation of cold molecular gas disks Junko Ueda…

1.Hertzsprung–Russell diagram LACC §16.2 16.3, 17.4 • Spectral Classes • Luminosity Classes • distribution; masses & lifetimes An attempt to answer the “big…

1.Typical Stellar EvolutionLACC §: 20.2, 21.4, 21.5 • Red Giant Branch• Horizontal Giant Branch• Asymptotic Giant Branch An attempt to answer the “big questions”:…

1. Henry Throop!! University of Pretoria ! &! Planetary Science Institute! Tucson, Arizona! ! Collaborators:! ! John Bally (U. Colorado)! Nickolas Moeckel (Cambridge)!…

1. PASJ: Publ. Astron. Soc. Japan , 1–??,c 2011. Astronomical Society of Japan. Propagation of Highly Efficient Star Formation in NGC 7000Hideyuki Toujima,1 Takumi Nagayama,2…

Chapter 16 Beyond Our Solar System 25.1 Properties of Stars  Star Color and Temperature • Color is a clue to a star’s temperature. A constellation is an apparent group…