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Documents Can Photo-Evaporation Trigger Planetesimal Formation? Henry Throop John Bally SWRI Univ.Colorado /.....

Slide 1Can Photo-Evaporation Trigger Planetesimal Formation? Henry Throop John Bally SWRI Univ.Colorado / CASA DPS 12-Oct-2004 Slide 2 Orion Nebula Photo-evaporation by extrnal…

Documents Accretion Disks around Stars and the Process of Planet Formation National Radio Astronomy...

Slide 1Accretion Disks around Stars and the Process of Planet Formation National Radio Astronomy Observatory The National Radio Astronomy Observatory is a facility of the…

Education Highly siderophile elements_in_earth_mantle_as_a_clock_for_the_moon_forming_impact

1.LETTER doi:10.1038/nature13172 Highly siderophile elements in Earth’s mantle as a clock for the Moon-forming impact Seth A. Jacobson1,2 , Alessandro Morbidelli1 , Sean…

Science Nebulae, quasars,

1.NEBULAE, QUASARS, AND BLAZARS Bryan Nozaleda 2. What is a nebula? A nebula, derived from the Latin meaning “mist,” is any cloud or collection of interstellar medium…

Documents Our Galaxy, The Milky Way

Ay 20 - Fall 2004 - Lecture 16 Our Galaxy, The Milky Way Our Galaxy - The Milky Way • Overall structure and major components • The concept of stellar populations •…

Documents The Origin of Oxygen Isotopic Anomalies Seen in Primitive Meteorites Edwin A. Bergin (U. Mich)...

Slide 1 The Origin of Oxygen Isotopic Anomalies Seen in Primitive Meteorites Edwin A. Bergin (U. Mich) Jeong-Eun Lee (UCLA) James Lyons (UCLA) Slide 2 Background: Oxygen…

Documents Can Photo-Evaporation Trigger Planetesimal Formation?

Can Photo-Evaporation Trigger Planetesimal Formation? Henry Throop John Bally SWRI Univ.Colorado / CASA DPS 12-Oct-2004 Orion Nebula Photo-evaporation by extrnal O and B…

Documents Kozai Migration Yanqin Wu Mike Ramsahai. The distribution of orbital periods P(T) increases from 120...

Kozai Migration Yanqin Wu Mike Ramsahai The distribution of orbital periods P(T) increases from 120 to 2000 days Incomplete for longer periods Clear excess at 3-4 days Evidence…

Documents Determination of the mass of black holes in active galaxies

Determination of the mass of black holes in active galaxies O. Marco ESO MBH vs host galaxy Active Galactic Nuclei (AGN) are powered by accretion of matter onto massive black…

Documents Chapter 15 The Formation of Planetary Systems

PowerPoint Presentation Chapter 15 The Formation of Planetary Systems 2 Astronomers routinely observe other young star systems, hoping to gain insight into the origins of…