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…
1. Science Centers and Planetaria as Citizen Science PlatformsWouter Schrier and Pedro RussoEU Universe Awareness / Leiden Observatory, the [email protected]…
Slide 1 Mariangela Bernardi UPitt/UPenn Galaxies Properties in the SDSS: Evolution, Environment and Mass Galaxies Properties in the SDSS: Evolution, Environment and Mass…
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…
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…
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…
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,…
PowerPoint Presentation Galaxy feedback in 3D Roberto Maiolino Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between…
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…