'10 myr' presentation slideshows

Lecture 7: Back into the Icehouse: Last 55 Myr (Chapter 6)

Lecture 7: Back into the Icehouse: Last 55 Myr (Chapter 6). CO2 evolution in the last 50 Myr. Did climate cool?. Cooling inferred from terrestrial evidences. Antarctic. Arctic. Northern mid-lattiude cooling inferred from leave shape. 10-15 o C. Problem with land records: incomplete,

446 views • 37 slides

Direct imaging of substellar objects around young and nearby stars: The SACY sample

481 views • 37 slides

Breakfast Talk: Views on Star Formation

Breakfast Talk: Views on Star Formation. Current Views on Star Formation. Francesco Palla INAF-Osservatorio di Arcetri, Firenze. 1. From clouds to stars: a unified scenario 2. Star Formation in clusters & associations: SF histories and accelerating SF

487 views • 36 slides

Theoretical SEDs in Starbursts: SFRs in both the UV and IR

334 views • 24 slides

High Contrast Spectral Imaging: the Case of GQ Lup

331 views • 20 slides

Placing Our Solar System in Context with the Spitzer Space Telescope

Michael R. Meyer Steward Observatory, The University of Arizona

300 views • 17 slides

Spitzer View of Massive Star Formation in the Magelanic Bridge

Spitzer View of Massive Star Formation in the Magelanic Bridge. Rosie Chen (University of Virginia) Remy Indebetouw , Karl Gordon, Greg Sloan, & the SAGE-SMC team. Motivation. Kennicutt (1998). Massive Stars -- energy source of the interstellar medium (ISM)

246 views • 11 slides