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Documents Galaxy feedback in 3D Roberto Maiolino. Feedback is the key: - reducing SF efficiency (gas...

Slide 1Galaxy feedback in 3D Roberto Maiolino Slide 2 Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between halo mass…

Technology Ecsite 2012 - Science Centers and Planetaria as Citizen Science Platforms

1. Science Centers and Planetaria as Citizen Science PlatformsWouter Schrier and Pedro RussoEU Universe Awareness / Leiden Observatory, the [email protected]

Documents Mariangela Bernardi UPitt/UPenn Galaxies Properties in the SDSS: Evolution, Environment and Mass...

Slide 1 Mariangela Bernardi UPitt/UPenn Galaxies Properties in the SDSS: Evolution, Environment and Mass Galaxies Properties in the SDSS: Evolution, Environment and Mass…

Documents Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen.

Slide 1 Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen Slide 2 Background Galaxies are full of stars, and sometimes gas and dust too. Beyond just images…

Documents Phil James Liverpool John Moores University Astrophysics Research Institute 22nd August 2007 STFC...

Slide 1 Phil James Liverpool John Moores University Astrophysics Research Institute 22nd August 2007 STFC PhD Summer School, Durham The Structure of Galaxies Slide 2 Talk…

Documents Physics 10, introductory lecture A. Albrecht January 2010.

Slide 1 Physics 10, introductory lecture A. Albrecht January 2010 Slide 2 Slide 3 Slide 4 Slide 5 Slide 6 Slide 7 The Keck 10m Telescopes on Mauna Kea, Hawaii Slide 8 Segments…

Documents Probing dark matter clustering using the Lyman- forest Pat McDonald (CITA) COSMO06, Sep. 28, 2006.

Slide 1 Probing dark matter clustering using the Lyman-  forest Pat McDonald (CITA) COSMO06, Sep. 28, 2006 Slide 2 The Lyman-  forest is the Ly  absorption by neutral…

Documents Is the Sodium Na D line useful?

Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen Background Galaxies are full of stars, and sometimes gas and dust too. Beyond just images & colors,…

Documents Galaxy feedback in 3D

PowerPoint Presentation Galaxy feedback in 3D Roberto Maiolino Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between…

Documents An Evolutionary Connection between AGNs and GALEX UV-excess Early-type Galaxies

An Evolutionary Connection between AGNs and GALEX UV-excess Early-type Galaxies Hyun-Jin Bae*, Kiyun Yun, Yumi Choi, and Suk-Jin Yoon Department of Astronomy and Center for…