'Gas disk' presentation slideshows

Lecture L12 ASTC25

Lecture L12 ASTC25. 1. Radiation pressure in action 2. Structures in dusty disks vs. possible reasons including planets 3. Dust avalanches, gas, and the classification of disks 4. Non-axisymmetric features without planets (dust avalanches) * * * 5. Pulsar planets

886 views • 73 slides

Debris disks

378 views • 37 slides

NUCLEI OF GALAXIES: First results/STATUS

373 views • 37 slides

Galaxy Evolution in the Virgo Cluster

Galaxy Evolution in the Virgo Cluster. Bernd Vollmer CDS, Observatoire de Strasbourg, France In collaboration with: P. Amram, C. Balkowski, R. Beck, A. Boselli, J. Braine, V. Cayatte, K. Chyzy, A. Chung, H. Crowl, W. Huchtmeier, J. Kenney, M. Marcelin, K. Otmianowska-Mazur, M. Soida,

380 views • 25 slides

Planet Formation with Different Gas Depletion Timescales: Comparing with Observations

Planet Formation with Different Gas Depletion Timescales: Comparing with Observations. Huigen Liu, Ji-lin Zhou, Su Wang huigen@nju.edu.cn Dept. of Astronomy Nanjing University Nanjing 210093, China. Previous works:. Core accretion scenario, Monte Carlo Method : Peering works:

326 views • 22 slides

PLANETARY MIGRATION in protoplanetary discs and OUTER SOLAR SYSTEM ARCHITECTURE

265 views • 22 slides

The Evolution of Protoplanetary Disks and the Diversity of Giant Planets

The Evolution of Protoplanetary Disks and the Diversity of Giant Planets. Extreme Solar Systems II September 2011 Ben Bromley Physics & Astronomy, University of Utah Scott Kenyon Smithsonian Astrophysical Observatory. Diversity of planets. the Solar System:

296 views • 17 slides

The Radial Profiles of Gas, Gas Metallicity and SFR in the SAMs for Molecular and Atomic Gas

The Radial Profiles of Gas, Gas Metallicity and SFR in the SAMs for Molecular and Atomic Gas. Fu Jian Max Planck Institute for Astrophysics, Garching 18/12/2012. Millennium and Millennium II Simulation. Millennium Simulation: Springel et al. 2005

317 views • 16 slides

Spiral Structure and Dynamics of NGC 5248

Spiral Structure and Dynamics of NGC 5248. D.C.C. Yen a , C.C. Yang b and C. Yuan a,b a Institute of Astronomy & Astrophysics, Academia Sinica, Taipei, Taiwan, R.O.C b Physics Department, National Taiwan University, Taipei, Taiwan, R.O.C.

204 views • 1 slides