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OBAMA OBAMA OBAMA Santiago, 7 Nov 2012

OBAMA OBAMA OBAMA Santiago, 7 Nov 2012

OBAMA OBAMA OBAMA Santiago, 7 Nov 2012. Multiplicity of Spectroscopic Binaries among Massive Stars: Origin and Implications on “Stergers” Hans Zinnecker SOFIA Science Center, NASA-Ames “Blue Stragglers” Workshop, Santiago. Slide 1 (why I am here )

By robert
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Cosmic Rays and Galactic Field

Cosmic Rays and Galactic Field

Cosmic Rays and Galactic Field. 3 March 2003 Astronomy G9001 - Spring 2003 Prof. Mordecai-Mark Mac Low. MHD waves. Robert McPherron, UCLA. Galactic Magnetic Field. Scale height Concentration by spiral arms. Dynamo Generation of Fields. Seed field must be present advected from elsewhere

By susandana (0 views)

AGB stars in Galactic Globular Clusters –

AGB stars in Galactic Globular Clusters –

AGB stars in Galactic Globular Clusters – Are They Chemically Distinct to Their Fellow RGB and HB Stars?. Simon Campbell. M5: SDSS. Collaborators. RSAA, Mt Stromlo, Australia: David Yong Elizabeth Wylie de Boer Monash University, Australia: John Lattanzio Richard Stanciffe

By kasi (141 views)

Young Stars In The Galactic Center

Young Stars In The Galactic Center

Young Stars In The Galactic Center. Audra K. Hernandez High Energy Astrophysics Discussion Group Friday 10th Feb. Topics of Discussion . Galactic Center Parameters What Kind of stars are there in the GC 2 rings of young stars Why is star formation hard at GC? Formation scenarios

By najwa (78 views)

Hypervelocity Stars Ejected from the Galactic Center

Hypervelocity Stars Ejected from the Galactic Center

Hypervelocity Stars Ejected from the Galactic Center. STScI Colloquium Oct 3, 2007 Warren R. Brown Smithsonian Astrophysical Observatory Collaborators: Margaret Geller, Scott Kenyon, Michael Kurtz. Radial Velocities from the MMT. The first “Hypervelocity Star”. Predictions. NY Times

By jontae (87 views)

Hypervelocity Stars Ejected from the Galactic Center

Hypervelocity Stars Ejected from the Galactic Center

Hypervelocity Stars Ejected from the Galactic Center. MMT Symposium June 14, 2006 Warren R. Brown Harvard-Smithsonian CfA Collaborators: Margaret Geller, Scott Kenyon, Michael Kurtz. The Milky Way. 30 kpc. 8 kpc. r=100 kpc. Kaufmann. The Galactic Center.

By ghazi (131 views)

Mass Loss from Galactic Bulge AGB stars

Mass Loss from Galactic Bulge AGB stars

Mass Loss from Galactic Bulge AGB stars. Margaret Meixner (STScI/ visiting Scientist at Harvard-Smithsonian CfA) Nimesh Patel, Dave Riebel, Ben Sargent, Sundar Srinivasan, Ken Young. Why Galactic Bulge?. Known Distance: 8 kpc (Reid 1993) Extreme environment

By dooley (171 views)

Galactic Magnetic Field Research with LOFAR

Galactic Magnetic Field Research with LOFAR

Galactic Magnetic Field Research with LOFAR. Wolfgang Reich Max-Planck-Institut für Radioastronomie Bonn, Germany. The Galactic magnetic field. What we want to know : - global field structure: disk + halo - regular/random component f(r) - field strength f(r) - field reversals

By finley (132 views)

Mass Loss from Galactic Bulge AGB stars

Mass Loss from Galactic Bulge AGB stars

Mass Loss from Galactic Bulge AGB stars. Margaret Meixner (STScI/ visiting Scientist at Harvard-Smithsonian CfA) Nimesh Patel, Dave Riebel, Ben Sargent, Sundar Srinivasan, Ken Young. Why Galactic Bulge?. Known Distance: 8 kpc (Reid 1993) Extreme environment

By cpickens (0 views)

Tracing Galactic structure with obscured luminous stars

Tracing Galactic structure with obscured luminous stars

Madrid March 2012. Tracing Galactic structure with obscured luminous stars. Ignacio Negueruela. Madrid March 2012. Tracing Galactic structure with obscured luminous stars. + High-mass stars in the infrared. Ignacio Negueruela. Francisco Najarro Artemio Herrero. Outline.

By lajos (105 views)

Chap 5: From Stars in Galactic Clusters to Stars in Fireworks

Chap 5: From Stars in Galactic Clusters to Stars in Fireworks

Chap 5: From Stars in Galactic Clusters to Stars in Fireworks. New Office hours Tuesdays 1:00 to 2:30 pm 2033 YH Exam on Friday Chapters 3, 4, 5 and 6.0-6.6 One page of notes Review Session Thursday Lec (1) 5:00 - 5:50 and Lec (2) 6:00 - 6:50.

By michael-stokes (138 views)